The galaxy appears as a well-defined elliptical object. It exhibits a relatively smooth, centrally concentrated light distribution, with minimal discernable substructure. The core region is bright and transitions gradually into a fainter halo. There's a slight elongation suggesting it is not perfectly spherical, and its shape can be approximated as oblate spheroid. The color profile suggests a population of older stars. No obvious spiral arms or dust lanes are visible, and there is no indication of any ongoing major merger activity or tidal disturbances. Overall, it appears to be a passively evolving, early-type galaxy.
