The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The central region exhibits a yellowish hue, suggesting a population of older stars. A faint, diffuse halo surrounds the central region, transitioning into a bluish color, potentially indicating the presence of younger stellar populations or ongoing, though possibly low-level, star formation in the outer regions. The overall structure appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions, although a slight asymmetry cannot be ruled out at this resolution. The galaxy's shape is predominantly oval, appearing more elongated than perfectly spherical.
