Dark matter (DM) is observed to correlate with regions of higher ordinary matter (OM) density, as DM's gravitational influence helps to pull OM together. However, this correlation is not absolute, as some areas may contain low-density DM without significant OM accumulation. DM is challenging to detect, primarily visible in high concentrations through phenomena like gravitational lensing, and it is suggested that maps may not show DM below certain density thresholds. The presence of DM is crucial for the stability of galaxies, preventing stars from escaping due to their velocities. Overall, DM is understood to permeate space, filling what was once considered empty.