The galaxy exhibits a generally smooth morphology, but with hints of possible features or a disk-like component. Its overall shape appears more intermediate than either perfectly round or elongated, leaning toward a flattened spheroid. There is a suggestion of a central bulge with decreasing luminosity outwards and a possible spiral structure contained within. There is a distinct color gradient that includes blue, green, and red, which could indicate areas of active star formation. The redder colors appear to exist in areas of the central bulge. The galaxy appears to be relatively undisturbed, but there is evidence of potential minor tidal interactions or internal activity, such as an asymmetry in the spiral arms.
