The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, fading gradually towards the edges, and is observed to be in between round and elliptical in shape. There's a suggestion of minor disturbances in its morphology; this might be due to a possible interaction or past merger event. There may be some ongoing low-level star formation based on what appears to be slightly bluer colors near the central region. Overall, the galaxy seems to be a fairly massive system with hints of recent, albeit subdued, activity.
