The galaxy presents as a fairly smooth, centralized structure with a high degree of overall symmetry. The light is concentrated in the center, which is bright and elliptical in shape. There is a distinct color gradient from the center, which is a yellowish-white, to the outer regions, which transition to a more bluish hue. This color variation suggests differing stellar populations and potential age gradients within the galaxy. The smooth appearance of the galaxy indicates that it is most likely an elliptical galaxy with minimal or no visible disk structure or spiral arms. The outer regions are diffuse and lack any prominent features, with only a slight hint of a more extended halo. There is no evidence of any major ongoing merger activity or strong tidal disturbances. Minor disturbances may be present. The galaxy is relatively round in shape, and its morphology suggests a more evolved system, having already undergone a significant amount of its star formation.
