The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, centrally concentrated light profile, with a gradual decrease in surface brightness towards the outer regions. The galaxy's color appears yellowish-white, suggesting a population of older stars. There is no obvious evidence of a distinct disk or spiral arms, nor is there any indication of ongoing major mergers or strong tidal disturbances. A subtle elongation is observed in the galaxy's shape, appearing slightly more rounded than cigar-shaped. Possible minor disturbance is present. The galaxy appears relatively isolated in its immediate vicinity.
