The galaxy presents an elliptical morphology, exhibiting a smooth, featureless structure. It appears nearly round, with a slight elongation. The light profile suggests a concentrated nucleus surrounded by a diffuse halo. Color gradients indicate a general trend from bluer hues in the outer regions to redder hues towards the core, with the outer regions displaying subtle disk-like colors. No significant signs of ongoing mergers or major disturbances are apparent, with little to no dust lanes or tidal features visible. The galaxy exhibits considerable luminosity.
