The galaxy presents a roughly elliptical morphology, appearing somewhat compact. The central region exhibits high luminosity, appearing bright white-blue. Surrounding the core, there is an orange-red band of light, with a blue haze extending outwards, suggesting a complex distribution of stellar populations and/or dust content. The presence of asymmetric features suggests possible ongoing interactions or internal disturbances. The smoothness and relative lack of distinct spiral arms or disk structure indicates a possible classification as an early-type or elliptical galaxy, although disturbances indicate it could be merging with another galaxy or undergoing structural changes.
