The galaxy presents a largely smooth, elliptical morphology with minimal discernible substructure. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness extending outwards. The color is generally consistent throughout the galaxy, appearing largely consistent with older stellar populations, though there may be some signs of recent star formation. There is no distinct disk component. The overall shape appears rather round. There is no immediately apparent evidence of ongoing major merger activity or strong tidal disturbances. The galaxy's appearance is consistent with it being a relatively undisturbed elliptical galaxy.
