The galaxy appears to be a relatively smooth, elongated elliptical galaxy, approximately 2.6 kpc in radius. It exhibits a somewhat cigar-shaped morphology, with no apparent spiral arms or distinct features indicating a disk-like structure. The color profile suggests an older stellar population, with a slight bluer hue toward the center indicating a central region of star formation. There is no evidence of any major ongoing mergers or significant tidal disturbances, but there could be minor disturbances present. The galaxy displays a relatively low star formation rate.