The galaxy presents a relatively smooth, elliptical morphology. There is very little disk-like structure apparent. The object appears nearly circular with a low likelihood of merging activity or major disturbances. The galaxy exhibits a concentrated central bulge region, with a radial falloff in luminosity toward its outer regions. The core appears significantly brighter with a blue-white color, while the outer regions tend to be a bit redder. This suggests a concentration of older stars within the extended halo of the galaxy, with ongoing but not very high rates of star formation. The overall features of the galaxy point to a fairly typical elliptical galaxy.
