The galaxy appears as a smooth, centrally concentrated object with an elliptical morphology. The light distribution transitions gradually from a bright, yellowish core to fainter, more diffuse outer regions. The galaxy exhibits a slightly elongated shape, appearing more "in between" than completely round or cigar-shaped. There are no visible signs of distinct spiral arms or a prominent disk structure. The overall appearance suggests a relatively undisturbed system, lacking any obvious tidal features or major disturbances indicative of recent merger activity. The observed color suggests a population of older stars, with moderate star formation occurring within.
