The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy with a notable central bulge. The light profile is highly concentrated, exhibiting a gradual decrease in surface brightness outwards from the core. The color is predominantly yellow-red, suggestive of an older stellar population, potentially with minimal ongoing star formation. The galaxy's shape is moderately elongated, not perfectly spherical, hinting at a possible disk component or triaxial structure. No prominent dust lanes or spiral arms are observed in the image. There is no apparent tidal debris or morphological disturbances indicative of recent major mergers. The galaxy appears to be relatively isolated.
