The galaxy appears as a singular, roughly circular, and relatively smooth structure. The light distribution is centrally concentrated, with a bright, yellowish core that diffuses outward into a more diffuse halo. The color suggests a population of older stars, and there isn't any evidence of spiral arms or a well-defined disk. There are some indications of a slight asymmetry or disturbance in the outer regions of the halo. Overall, the morphology is consistent with an elliptical or lenticular galaxy.
