The galaxy presents as a somewhat diffuse object, exhibiting an elliptical morphology with a relatively smooth profile, although there is evidence of substructure within. There's a discernible bulge component, roughly centralized within the galaxy's overall structure. The light distribution appears centrally concentrated, with a gradient of decreasing brightness moving outwards. The galaxy exhibits a gold color, potentially indicative of a population of older stars. The outer regions of the galaxy appear fainter and more spheroidal in shape. Faint light suggests there may be a very weak spiral structure, although the image resolution makes it difficult to discern conclusively.
