The galaxy presents as a single, centrally concentrated luminous object. It exhibits a smooth morphology without discernible spiral arms or a prominent disk structure. The central region appears bright and yellow, suggesting an older stellar population. The galaxy has an elliptical shape, with a moderate degree of elongation. There are no visible signs of recent mergers or tidal disturbances affecting its overall structure. The outer regions gradually fade into the background, indicating a smooth density profile.
