The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, which graduates into a diffuse halo. The color profile suggests a population of older stars. The galaxy's apparent roundness indicates it is likely viewed close to face-on. There is no obvious spiral arm structure or significant dust lane obscuration visible. No signs of major merger events are observed, and the galaxy appears relatively undisturbed. Based on its redshift, this is a relatively distant galaxy.
