The galaxy presents as a largely featureless elliptical morphology, with a bright, concentrated core. There is little discernible structure or detail in the surrounding halo. Color gradients suggest a population of older stars, evidenced by the reddish-yellow hue that diminishes from the core. The galaxy appears to be relatively isolated, without obvious signs of interaction or tidal disturbances from nearby galaxies. Its round appearance indicates it is most likely an elliptical. Star formation seems to be low. The galaxy exhibits a smooth profile.
