Caption: "Projected density plot of a cosmological redshift z = 2.5 dark halo from a cosmological N-body simulation. The visible part of the galaxy (NOT shown in the image) lies at the dense center of the dark halo and has a diameter of roughly 20 kiloparsecs. There are also many satellite galaxies, each with its own subhalo which is visible as a region of high dark matter density in the image." (Slightly edited.)
The image is false color---but you knew that, right?
The dark matter itself is believed to consist of a swarm of exotic particles whose nature we do NOT yet know.
Almost the only effect of the exotic particles is through their gravity.
They are extremely unreactive via other fundamental forces with themselves or anything else.
The dark matter particles form a kind of gas, but NOT an ordinary gas since they barely interact.
They just move around in chaotic orbits which is why they can be modeled by N-body simulations.
If they were hot dark matter (i.e., relativistic matter), they would NOT have clump together to have helped form galaxies.
Cosmic neutrinos form at least a part of the hot dark matter of the observable universe, but at present they seem to have little effect on cosmic evolution.
Maybe the cold dark matter consists of primordial black holes.