The galaxy exhibits a generally elliptical morphology. The core region appears bright and concentrated, with a smooth, diffuse halo extending outwards. There is a faint disc visible and some indication of potential disturbances to this shape. The color gradient suggests a predominantly older stellar population. The redder regions appear to be associated with the central bulge, while the disc region has a slightly bluer tint, potentially indicating more recent star formation or a different stellar population. There is no strong indication of a clear spiral structure, rather the faint hints of a disc.
