The galaxy appears as a centrally concentrated, elliptical or lenticular system with a smooth, featureless morphology. The object exhibits a moderate ellipticity, leaning towards an "in-between" form rather than perfectly round or highly elongated. There is no evidence of spiral arms, bars, or significant dust lanes. The galaxy's color index suggests a relatively evolved stellar population. The light is dominated by older stars. No obvious signs of tidal disturbances, strong interactions, or active galactic nuclei are apparent in this imaging, supporting its classification as a quiescent system. There may be very minor star formation present. Overall, the galaxy seems to be an isolated, relatively undisturbed system undergoing minimal recent activity.
