The galaxy presents an elliptical morphology, exhibiting a centrally concentrated bulge with a smooth light distribution. The core region appears yellowish, indicative of an older stellar population. A faint, diffuse halo surrounds the central bulge, extending outwards with a slightly elongated shape. There are hints of a very faint disk or spiral arms that appear tightly wound, appearing more as extensions of the smooth halo rather than well-defined structures. There does not appear to be strong evidence of recent or ongoing major merger activity in this galaxy.
