The galaxy presents as a relatively smooth and elliptical-like morphology. It exhibits a centrally concentrated bulge, which appears bright and dominates the overall light profile. The outer regions of the galaxy fade gradually, with no readily discernible spiral arm structure. The galaxy exhibits a slightly elongated shape, suggesting a modest degree of ellipticity. There appears to be some color variation, with the central bulge exhibiting a yellower hue, which is consistent with an older stellar population. The outer regions appear slightly bluer, perhaps indicative of more recent star formation, though this is subtle. There is no apparent major disturbance or merging activity.
