The galaxy presents as a largely featureless, elliptical-like structure. It exhibits a centrally concentrated brightness profile, with luminosity decreasing smoothly and gradually from the core outwards. The central region appears yellowish, possibly indicating an older stellar population or dust obscuration. There is minimal evidence of spiral arms, bars, or any distinct morphological features typically associated with disk galaxies. Its round shape suggests a classification toward the E0-E3 range on the Hubble sequence, with a possible slight deviation from perfect sphericity. No obvious tidal features or signs of recent mergers are observed in the immediate vicinity. The galaxy appears relatively isolated, showing no strong interactions with other galaxies in the field. The outer regions of the galaxy become increasingly faint, blurring into the background sky. Overall, the galaxy presents as a fairly typical, quiescent elliptical galaxy.
