The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular galaxy. It exhibits a noticeable radial gradient in surface brightness, with a bright, unresolved core diminishing outwards to a faint, diffuse halo. There are hints of spiral arm structure, but they are faint and largely indistinct. Color gradients suggest the presence of older stellar populations dominating the central regions, with potentially bluer, younger stars at the outer edges. No clear dust lanes or other distinct morphological features are apparent, although some minor disturbances might be present. The galaxy exhibits an overall round morphology with a slight elongation. There are no signs of any major mergers occurring, but there are a few minor disturbances present.
