The galaxy presents as a yellowish-white, relatively compact structure, suggestive of an elliptical or lenticular morphology. The central region appears bright and diffuse, lacking distinct features such as spiral arms or a prominent bulge. The outer regions fade gradually, indicating a smooth transition in stellar density. There is some evidence of possible tidal disturbances or interactions as there are some asymmetric features that point to possible mergers. The overall color suggests an older stellar population.
