The galaxy appears as a centrally concentrated system, likely an elliptical, with a smooth light distribution. The core exhibits a yellowish-white hue, potentially indicating an older stellar population. A subtle gradient towards bluer colors can be observed in the outer regions, possibly suggesting the presence of younger stars at the outskirts, although this is less pronounced. The overall structure is generally round, with a possible slight elongation. There are no obvious signs of strong tidal interactions or major disturbances in the galaxy's shape, although a very subtle asymmetry cannot be ruled out. No spiral arm features or prominent dust lanes are visible.
