The galaxy presents a generally smooth and elliptical morphology. The central bulge is prominent, displaying a concentrated luminosity gradient. A subtle disk-like structure appears to surround the central region, though it lacks distinct spiral arm features. The galaxy exhibits a color gradient, with the core appearing more yellow and the outer regions trending toward redder hues. There is no obvious evidence of major mergers or significant tidal disturbances, but a slight asymmetry cannot be ruled out. Star formation appears to be generally quiescent, with little evidence of recent or ongoing activity. The overall appearance suggests a relatively evolved stellar population dominating the observed light.
