The galaxy presents as a roughly elliptical structure. Its core exhibits a bright, concentrated luminosity, appearing yellow-white. Moving outwards from the core, the luminosity gradually diminishes. The outer regions display a bluer hue, indicating the presence of younger stellar populations. There's a subtle hint of a disk-like structure surrounding the central bulge. The overall appearance suggests a galaxy undergoing a relatively low rate of star formation. There does not appear to be any signs of significant disturbances or major mergers occurring.
