The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated luminosity profile. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Progressing outward, a gradual transition to a bluer color is observed in the surrounding halo. The galaxy displays a nearly circular morphology, with no apparent signs of strong tidal distortions or major mergers. Minimal indications of spiral arm structure or a prominent disk are evident in the image. Faint hints of potential minor disturbances are present, but these are not pronounced. The overall impression is that of a mature galaxy with a dominant spheroidal component.
