The galaxy presents a primarily smooth morphology, with an apparent dominance of spheroidal structure. The central region exhibits a concentrated, bright, yellowish-white luminosity, indicative of an older stellar population. There is a possible disk with some arms or plumes of fainter, reddish material extending away from the central bulge, appearing somewhat disturbed. There seems to be a tidal tail or possible merger. The overall color suggests a relatively evolved system, possibly an elliptical galaxy or a spiral galaxy with a prominent bulge and subdued star formation.
