The galaxy presents as a relatively bright, elliptical structure with a smooth, centrally concentrated bulge. The core region exhibits a bright yellowish-white hue, suggesting a population of older, less massive stars. Moving outward from the core, a distinct color gradient is observed with the surrounding region displaying a bluish tint. This suggests the presence of a younger stellar population and potentially ongoing, though subdued, star formation within the outer regions. The overall shape is somewhat elongated but appears more or less regular, showing no obvious signs of significant tidal disturbances or ongoing major mergers. Subtle, diffuse arms or disk-like structures are faintly visible extending from the central region, but they do not appear well-defined. The galaxy does not appear to be particularly massive.
