The galaxy presents as a centrally concentrated system, with a smooth, diffuse light profile. There is a noticeable color gradient, shifting from a yellowish hue in the core to a bluer, fainter outer region. No distinct spiral arms or bar structures are apparent, suggesting a more spheroidal or elliptical morphology. A slight asymmetry or subtle feature is detected on one side, potentially indicating a minor interaction or disturbance. Overall, the galaxy appears relatively undisturbed, with a well-defined but somewhat fuzzy boundary. Its color suggests a mixed stellar population, with older stars dominating the core and younger stars scattered throughout the halo.
