The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical or lenticular given the lack of discernible spiral arm structures. The light distribution is smooth and falls off gradually from the core. It exhibits a high degree of circularity. There is no clear evidence of ongoing major mergers or strong tidal disturbances in this image, nor is there evidence of prominent dust lanes. Overall, the galaxy appears to be a relatively undisturbed system. There is a subtle color gradient from the center outwards, suggestive of differing stellar populations with the center potentially hosting older stars or a more metal-rich population.
