The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, surrounded by a more diffuse halo. The central region appears yellowish, suggesting a population of older stars. There is some indication of bluer components, possibly linked to younger stellar populations or star forming regions, as the area slightly further out from the center has a bluish tint. The overall shape appears to be neither perfectly spherical nor highly elongated. The presence of some irregularities in the morphology cannot be discounted at this resolution, suggesting possible minor interactions or internal disturbances. There are hints of disruption and possible star formation. The galaxy doesn't seem to show any sign of a major ongoing merger.
