The galaxy presents as a singular, relatively smooth object with a high degree of circularity. There are no immediately apparent spiral arms or a distinct disk structure. The light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer edges. Subtle variations in color are observed, transitioning from a bluish-white core to more red hues towards the periphery. This could be due to differing stellar populations or dust extinction. There is no evidence of tidal tails, ongoing mergers, or significant morphological disturbances.
