The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated central region, likely indicating a significant concentration of stars and possibly a supermassive black hole at its core. The galaxy appears to be fairly rounded, with a lack of prominent spiral arms or distinct disk features. There is a subtle color gradient, with the central bulge appearing more reddish or yellow, transitioning to a slightly bluer or greener hue in the outer regions. This suggests a possible difference in stellar populations, with older, redder stars dominating the center and younger, bluer stars present in the surrounding areas. No major signs of ongoing merging or significant tidal disturbances are readily apparent, implying a relatively quiescent state. The galaxy's overall appearance is consistent with that of a massive galaxy with moderate star formation.
