This galaxy presents as a relatively smooth, centrally concentrated object, potentially elliptical in morphology. The core exhibits a distinct yellow-orange hue, suggestive of an older stellar population dominating the central region. Moving outwards, the light profile gradually diminishes. There is some indication of a very faint, diffuse halo. The overall shape appears nearly round with some mild disturbances of matter around the object, but no signs of major mergers or prominent tidal features are discernible. Given the colour profile, it is possible that the galaxy is currently undergoing some level of star formation in the outer regions.
