The galaxy presents as a concentrated, elliptical morphology, displaying a notably smooth light distribution. The central region exhibits a bright, yellowish-white core that fades outwards into a diffuse halo. There are no immediately discernible spiral arm structures or prominent dust lanes. The overall shape tends towards round, with a slight elongation suggestive of an elliptical galaxy. The galaxy appears isolated, with no visual evidence of major disturbances or mergers. Subtle indications of a minor gravitational interaction are not entirely excluded, based on a mild asymmetry in the outer halo.
