The galaxy appears to be elliptical in morphology, exhibiting a generally smooth, round structure with minimal discernible features. A concentrated, bright core region dominates the galaxy's luminosity, with a gradual decrease in brightness toward the outer edges. The color profile suggests an aging stellar population, with a yellowish-red hue dominating the central bulge. There is a faint indication of blue-ish star formation in the very outer regions. The object shows no signs of major tidal disturbances or ongoing mergers, and no distinct spiral arm structure is visible. Overall, the galaxy's characteristics point toward a system dominated by older stars with a relatively low rate of ongoing star formation, but not zero.