This galaxy presents as a primarily smooth, centrally concentrated object with a relatively round morphology. The light distribution indicates a bulge-dominated system. There is some suggestion of a slight disturbance in the outer regions, potentially indicative of minor interactions or past mergers. The galaxy displays a color gradient, with the central bulge appearing yellower compared to the slightly bluer outskirts. Overall, the galaxy appears to be relatively evolved with a moderate amount of ongoing star formation.
