The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge which transitions smoothly into a fainter, more diffuse halo. There is no evidence of spiral arm structure or a distinct disk. The light distribution indicates a high degree of rotational symmetry, with an axial ratio close to unity. Color gradients suggest a slightly bluer center, indicating younger stellar populations concentrated towards the core. Overall, it presents as an early-type galaxy with limited recent star formation.
