The galaxy presents as a concentrated elliptical form, exhibiting a smooth, centrally-concentrated light profile. The core region appears bright and yellowish, indicating a possible concentration of older stellar populations. There is a subtle flattening of the galaxy's shape; it is not perfectly spherical, but rather leans slightly towards a flattened spheroid. The outer regions of the galaxy gradually fade into the background, displaying a diffuse and faint halo. Subtle disturbances or minor interactions are possibly indicated by slight asymmetries in the outer regions, yet these are minimal. Overall, the galaxy's structure indicates a relatively evolved system with a likely substantial stellar mass.
