This galaxy presents as a moderately bright, well-defined elliptical object. The central region exhibits a smooth, concentrated luminosity profile, suggesting a high stellar density. The isophotes appear generally round, with a slight elongation along a north-south axis. A faint, diffuse halo surrounds the central bulge, gradually fading into the background sky. No distinct spiral arm structures are visible, and there is minimal evidence of dust lanes or prominent star-forming regions. The overall color appears relatively uniform across the galaxy, with a subtle blue tint, implying a moderate population of younger stars, with some indication of ongoing, albeit low, star formation activity. There are no apparent signs of major mergers or significant tidal disturbances, but some minor disturbances may be occurring.
