The galaxy presents as a generally smooth, elliptical-like structure. There is a high concentration of light towards the center, diminishing outwards. The central region appears nearly spherical and is bright yellowish-white, indicating older stellar populations. The outer regions are less bright, but seem to have some disk like features. There is no evidence of spiral arms or significant dust lanes. The galaxy's overall color suggests it's a relatively evolved system, perhaps a lenticular galaxy, with ongoing star formation. It exhibits a high Sersic index suggesting the central bulge dominates the light profile.
