The galaxy presents a predominantly smooth appearance with a centrally concentrated luminosity. A subtle disk-like structure may be present, although it is not a clearly defined spiral or barred spiral. There are some faint structural features, suggesting some level of disturbance. Color gradients are evident, with a bluer core region transitioning to redder outer regions. The overall color index suggests that the galaxy is likely undergoing some level of star formation, albeit at a relatively low rate. Morphologically, the galaxy does not show signs of a major merger. There may be signs of a minor merger or other tidal disturbance visible.
