The galaxy presents as an elliptical morphology, with a smooth and concentrated light profile. The central region exhibits a yellowish-white hue, suggesting a population of older stars, while the outer regions display a slightly bluer color gradient. There is a subtle indication of disk-like structure, but the dominant feature is the smoothness of the light distribution. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. It has a moderate inclination. Overall, the galaxy appears to be a relatively massive system, potentially with suppressed recent star formation.
