The galaxy presents as a generally smooth, elliptical-like structure. The light distribution suggests a concentration of older stellar populations within the central region, which appears yellowish. The galaxy is somewhat elongated. There is faint evidence of a disk-like component or spiral arm structure. Overall, the galaxy appears relatively undisturbed, without signs of major merger events or significant tidal distortions. There is a degree of asymmetry to the outer regions, suggesting possible minor interactions or disturbances.
