The galaxy presents as a centrally concentrated elliptical morphology. The core exhibits a bright, yellowish-white hue, indicating a likely older stellar population. Moving outward from the core, the light profile gradually diminishes, with the outer regions displaying a bluer tint. This suggests the presence of a younger stellar population in these areas, though considerably less dominant than the older core population. Overall, the galaxy appears relatively smooth, with no prominent dust lanes or spiral arm structures visible. There is a slight elongation of the galaxy along one axis, suggesting a moderate degree of ellipticity. No signs of ongoing major mergers are readily apparent in the image. Faint hints of tidal disturbances may be present, however.
