The galaxy appears as a relatively smooth, centrally concentrated object with a generally elliptical morphology. A dominant, roughly circular component constitutes the primary body of the galaxy. Its color profile indicates an older stellar population, with a yellow-orange hue suggestive of evolved stars and a low rate of recent star formation. Possible signs of a minor disturbance or interaction are present, perhaps indicating an ongoing or recent merger event. The galaxy exhibits a faint, diffuse halo that may be indicative of tidal debris or a broader distribution of older stars.
