The galaxy presents as a centrally concentrated object with a smooth overall morphology. It exhibits an elliptical or lenticular shape, appearing elongated but lacking distinct spiral arm structures. A prominent central bulge dominates the galaxy's luminosity, with a yellowish hue suggesting an older stellar population. The outer regions appear fainter and more diffuse, with a slight bluish tint possibly indicating the presence of some younger stars or ongoing star formation at a low level. There is no apparent evidence of tidal features, major disturbances, or ongoing merging activity. The galaxy's disk appears relatively undisturbed.
