The galaxy presents as a roughly elliptical, spheroidal structure, exhibiting a smooth and centrally concentrated morphology. Its light profile suggests minimal substructure. The galaxy appears quite round. Color gradients within the galaxy are subtle, trending towards redder hues in the central regions, indicative of an older stellar population. There is no clear evidence of spiral arms, a disk, or ongoing major merger activity, but a slight asymmetry cannot be ruled out. Star formation appears very low. The estimated size corresponds to an average sized galaxy.
