The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a yellowish hue, potentially indicating an older stellar population. There is a subtle gradient from the brighter, yellowish core to a fainter, reddish outer region. No distinct spiral arms or disk-like features are discernible within the observable structure. The overall form suggests an evolved system. There is no noticeable presence of dust lanes or significant star-forming regions. The object appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers.
