The galaxy presents a generally smooth and centrally concentrated morphology. The light distribution appears relatively even, with a dominant, bright central region that fades gradually towards the outer edges. There are no prominent spiral arms or a well-defined disk structure visible. It exhibits a round appearance. The color profile suggests a population of older stars, indicated by the yellowish hue in the central region, possibly accompanied by some ongoing star formation, as hinted by the slightly bluer outer regions. Overall, the galaxy appears relatively undisturbed, showing no clear signs of recent major mergers or tidal interactions, although a minor disturbance is possible. Its estimated size indicates it's a substantial galaxy.
