The galaxy appears as a single, relatively smooth, and round object. There is a concentrated central bulge, with the light appearing more yellow and dense. The outer regions of the galaxy show a more diffuse halo of blue light, suggesting some ongoing star formation. There are no readily apparent spiral arms or bars. The overall morphology is consistent with an elliptical galaxy, exhibiting a high degree of central concentration with a smooth light profile. There is no evidence of major disturbances or ongoing merging activity, based on the symmetric distribution of the light.
