The galaxy appears as a centrally concentrated, largely spheroidal object. Its color is primarily yellow-orange, suggesting a dominant population of older stars and a lower rate of on-going star formation. There is little evidence of spiral arm structure or significant dust lanes. The smooth, rounded morphology points towards it being a relatively undisturbed system. The galaxy presents as a single, coherent entity, with no apparent signs of major mergers or tidal distortions. Overall, it is a relatively compact, evolved system that is not experiencing a high rate of star formation.
