The galaxy presents as an elliptical system with a moderately smooth light distribution. The central region exhibits a bright, concentrated core, suggestive of a supermassive black hole. There is a subtle color gradient, with the core appearing more yellow-orange. The outer regions of the galaxy fade gradually into the background, exhibiting a slightly flattened shape. There is no apparent spiral structure or significant dust lane obscuration. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interaction or ongoing merger activity, though there are some signs of minor disturbance of the morphology, but nothing that is readily visible.
