The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely round with some deviation. There is no clear evidence of spiral arms or a distinct disk-like structure. The galaxy's light is dominated by a central bulge that gradually fades outward. There is a suggestion of minor disturbances in the outer regions of the galaxy, possibly indicating past interactions or accretion events, but it mostly appears undisturbed. The overall color suggests an older stellar population, with no exceptionally strong blue or red features dominating.