The galaxy presents as a somewhat diffuse, centrally concentrated elliptical or lenticular system. It exhibits a smooth, largely featureless morphology, lacking prominent spiral arms or significant dust lanes discernible at this resolution. The overall color appears reddish, indicative of an older stellar population and potentially suggesting suppressed star formation activity. There is a slight elongation to the galaxy's shape, which could indicate a mild interaction or tidal disturbance but is inconclusive. The light profile suggests a moderate size for this type of galaxy, with a relatively compact core transitioning to a more extended halo.
