The galaxy presents as a roughly elliptical object with a smooth, largely featureless appearance. The central region exhibits a concentration of light, surrounded by a more diffuse halo. The color gradient suggests a redder core transitioning to bluer outer regions, which would be indicative of older stellar populations concentrated in the center, with relatively younger stars populating the edges. There are hints of minor disturbances, perhaps due to a past or ongoing interaction. The morphology is predominantly smooth, with some evidence of a disk.
