The galaxy presents as a centrally concentrated, luminous object with a generally smooth morphology. It appears nearly circular in projection, exhibiting high degree of rotational symmetry. There is a distinct central bulge, with intensity decreasing radially outward. The colour profile indicates a population of older stars. There is no apparent evidence of spiral arm structure or significant dust lanes. The overall structure and lack of prominent features suggest a relatively evolved system with little to no ongoing major mergers or interactions. The subtle colour variations present might indicate recent minor disturbances.
