The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth light distribution indicative of an elliptical morphology. The core is bright and yellowish-white, with color gradients suggesting older stellar populations dominating the center. Fainter, more diffuse regions extend outward from the core, these outer regions appear slightly bluer in color, possibly suggesting some younger star formation. The overall shape appears largely spheroidal, but there is a slight flattening or elongation along one axis. No distinct spiral arms or strong dust lanes are visible. Evidence for any significant ongoing mergers or tidal interactions is not readily apparent.
