The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region is bright and compact, displaying a yellowish-white hue. Extending outwards from the core is a more diffuse halo. The overall shape is somewhat elongated, leaning towards an in-between, not highly rounded, form. There is a suggestion of a subtle disk-like structure. There isn't any visible evidence of major disturbances or ongoing merger activity, although minor disturbances cannot be ruled out. Color gradients indicate possible variations in stellar populations, with bluer tones present in the outer regions. The overall color profile suggests the presence of both young and old stellar populations.
