The galaxy presents as a flattened, disk-like structure, approximately 12 arcseconds in diameter. The central region exhibits a bright, concentrated core, suggesting a possible active galactic nucleus or a dense stellar population. A faint spiral arm structure is suspected to be present but the arms are disrupted. The galaxy's overall color appears to be a pale blue-green, with some regions appearing more red, potentially indicating variations in stellar populations or dust content. The disk of the galaxy shows signs of asymmetry and tidal disturbances, potentially indicative of an ongoing or recent merger event. A prominent artifact is seen obscuring the galaxy.
