The galaxy presents as a fairly smooth elliptical or lenticular structure. The overall color is reddish-orange, suggesting a population of older stars and a low rate of current star formation. There's minimal evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions, though there may be a minor asymmetry suggesting a possible past interaction. The light profile seems fairly concentrated towards the center, with a gradual decrease in intensity outward. Based on color and morphology, this galaxy likely resides on the red sequence.