The galaxy appears to be a relatively smooth elliptical galaxy with a noticeable central bulge. It exhibits a concentrated luminosity profile, where the brightness rapidly decreases from the center outwards. The color profile suggests an older stellar population, with a yellowish-red hue dominating the galaxy's overall appearance. There is no apparent disk structure, spiral arms, or significant dust lanes. The galaxy's shape appears close to elliptical, with no apparent major disturbances. The overall appearance indicates a gravitationally relaxed system that has likely undergone significant merging events in the past, resulting in a relatively homogeneous stellar distribution.
