The galaxy presents a generally smooth, elliptical appearance with a high degree of circularity. The light distribution is centrally concentrated, exhibiting a strong bulge component. There is no readily discernible disk structure, nor are there any prominent spiral arms or bar features visible. The galaxy's color appears primarily yellowish-orange, suggesting a population of older stars and a low rate of ongoing star formation. There is no evidence of active galactic nucleus activity or significant dust lanes. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions in this image. There may be some faint, minor asymmetry in the outer isophotes, potentially indicative of a past minor merger event. Overall, it seems to be a relaxed system.
