The galaxy exhibits a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The color gradient suggests an older stellar population, with a reddish core indicating a concentration of evolved stars and dust. The outer regions show a slight bluer tint, hinting at some ongoing, albeit minimal, star formation activity. There is no obvious sign of an active galactic nucleus, tidal tails, or significant interactions with neighboring galaxies. The overall appearance points to a galaxy that is relatively relaxed and dynamically settled. The round shape supports this. There is no evidence of a major merger in recent history. The color profile and morphology are consistent with a massive galaxy.