The galaxy appears as a centrally concentrated, elliptical-like structure. There is a bright, yellowish-orange core, indicating a concentration of older stars. The galaxy exhibits a smooth, diffuse halo extending outwards from the core, with a gradual decrease in luminosity. Hints of bluer regions are observed within the halo, possibly suggesting areas of more recent star formation. The overall form suggests a system with minimal ongoing merger activity. There is no apparent spiral structure. The galaxy appears to be relatively isolated.
