The galaxy presents as a relatively smooth, elliptical form. Its central bulge is quite prominent and appears nearly spherical, exhibiting a concentrated luminosity gradient towards the nucleus. The outer regions of the galaxy, transitioning into the halo, show a gradual decrease in brightness. There is a subtle hint of disk-like structure, but it's not particularly distinct. The overall color profile suggests a red-sequence galaxy, likely dominated by an older stellar population, though there are subtle color variations within the galaxy that could indicate some ongoing, albeit limited, star formation, or perhaps dust lanes. The object does not appear to be undergoing any major merging events, though a slight asymmetry might suggest a minor past interaction.
