Caption: Artist's conception on a quasi logarithmic scale of the observable universe (that part of the universe inside of our past light cone). Going outward from the center at the Sun, are the Solar System inner planets, the Solar System outer planets, the Kuiper belt, the Oort cloud, Alpha Centauri, the Perseus Arm, the Milky Way, the Andromeda galaxy (M31, NGC 224), nearby galaxies, the large scale structure (which is sometimes now called the cosmic web), the cosmic microwave background (CMB), and the Big Bang's invisible plasma on the edge.
Features:
Note the original cosmic background radiation at the recombination era (∼ 378,000 years after the Big Bang) that evolved to be CMB (which is invisible in the visible band (fiducial range 0.4--0.7 μm)) had a blackbody radiation temperature of ∼ 3000 K (Wikipedia: Cosmic microwave background: Relationship to the Big Bang), and so would have looked white hot or maybe even blue hot to the human eye (see Wikipedia: Red heat).
Note the comoving radius of the observable universe is a true physical distance: i.e., one measurable at an instant in time with a ruler. But, in fact, we CANNOT measure it with a ruler. It is NOT a direct observable and its value can only be determined from a cosmological model.
What is the large enough scale? Circa 2023, a commonly suggested value for the cosmological principle scale is ∼ 400 Mpc = 0.4 Gpc (see Wikipedia: Cosmological principle: Observations).
Since 0.1 Gpc is much less than comoving radius of the observable universe = 14.25 Gpc = 46.48 Gly (current value), we can see the average behavior of the observable universe and our view of it should be typical (which as a hypothesis is called Copernican principle).
Everyone (i.e., us humans and the aliens) from their observing stations should see the same observable universe when averaged on a large enough scale.
So it looked different in the past. And we actually see it looking different due to the finite vacuum light speed c = 2.99792458*10**8 m/s.
The farther, we look out, the farther we look back in cosmic time. The time difference between now and when a light signal started out toward us is the lookback time.
So cosmologists have it over historians: cosmologists can actually see the past---the average past, NOT the past of where we are in the observable universe: i.e., in the Milky Way in the Local Group in the Virgo Supercluster in the Laniakea Supercluster.