The galaxy appears as a largely featureless, elliptical or spheroidal structure with a smooth light profile. It exhibits a concentrated core, with a diffuse halo of luminosity extending outwards. The color indices suggest a population of older stars, with a relatively small population of younger stars. There is no discernible spiral arm structure or dust lane visible, further indicating an elliptical classification. No signs of any recent major merger events are evident in the morphology, though some minor tidal disturbances cannot be ruled out. The galaxy appears to be relatively isolated in its immediate environment.
