The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated, spheroidal structure with a high degree of symmetry. No distinct spiral arms or prominent disk features are discernible, supporting a classification as an elliptical galaxy. The color is relatively uniform, with a slight reddish-yellow hue indicative of an older stellar population and a reduced rate of ongoing star formation. There is no evidence of significant tidal disturbances or ongoing mergers.
