The galaxy presents a smooth, elliptical morphology. It exhibits a centrally concentrated bulge with a gradual decrease in luminosity towards the outer regions. The light distribution suggests a relatively high Sersic index, indicating a steep concentration of light in the core. The apparent axial ratio indicates the galaxy is somewhat flattened, but not highly elongated. There is a faint suggestion of a disk-like structure but it appears quite small. Colors are indicative of a galaxy with evolved stellar populations. Faint star formation may be taking place.