The galaxy presents as a fairly luminous, elliptical system. It exhibits a high degree of central concentration, with the light intensity diminishing smoothly outwards from a bright, compact core. The overall morphology is quite smooth, lacking prominent spiral arms or other distinct features usually associated with disk galaxies. The galaxy appears largely spheroidal in shape, with only a slight deviation from perfect circularity. There is no obvious dust lane or other obscuring material visible. Subtle color gradients may be present, with the core appearing somewhat bluer than the outer regions, hinting at potential variations in stellar populations or recent star formation activity, though low current star formation is likely. No signs of tidal disturbances or ongoing mergers are apparent. The light is dominated by older stellar populations.