The galaxy presents as a relatively smooth, rounded structure. The galaxy exhibits a concentrated central bulge with a diffuse halo, indicative of an elliptical morphology. Color gradients suggest a population of older stars, particularly within the central regions. There is an apparent lack of significant dust lanes or spiral arm structures. Minor asymmetries or disturbances cannot be ruled out due to the image resolution. Overall the light distribution appears relatively uniform, with no immediately obvious features indicative of recent or ongoing major merger activity.