The galaxy presents as a somewhat diffuse object, generally elliptical in shape. Its core appears relatively bright and concentrated, exhibiting a yellowish-white hue, which may indicate a population of older stars. Emanating from the central region is a more faintly illuminated halo of light. There are potential indications of disturbances in its overall structure and morphology. A significant fraction of the galaxy's light appears concentrated in one general area, although it does not exhibit a clear spiral or bar structure. There is a suggestion of interacting components or tidal debris, hinting at a possible past or ongoing merger event with another galaxy.
