The galaxy presents as a somewhat elliptical, but nearly circular, object with a smooth appearance. It exhibits a prominent, bright central bulge that gradually fades into a more diffuse halo. There is some indication of minor disturbances in the surrounding region, perhaps indicative of a past merger or tidal interaction. Color gradients suggest a generally older stellar population, especially concentrated in the central region. Despite its overall smooth morphology, there is a hint of a disk-like structure within the outer regions of the halo.
