The galaxy exhibits a centrally concentrated luminosity profile, appearing largely smooth and elliptical in shape. A bright, yellowish core region is evident, suggesting a concentration of older stellar populations. Extending outward from the core, the light fades gradually, exhibiting a diffuse halo. There is a subtle suggestion of some substructure or minor disturbance. It's shape appears slightly rounded, but not perfectly spherical. There is no evidence of a distinct disk component or spiral arm structure. Overall, the galaxy appears to be relatively undisturbed, with only subtle hints of interactions. The lack of prominent blue regions suggests a relatively low ongoing star formation rate.
