The galaxy appears as a singular, concentrated object with a generally elliptical morphology. The light distribution is relatively smooth, suggesting minimal substructure. There is a slight color gradient observed within the galaxy, with the central regions appearing more yellow-red, potentially indicating an older stellar population. The outer regions exhibit a marginally bluer hue, suggestive of possible recent or ongoing star formation, albeit at a relatively low rate. There is no obvious evidence of a prominent disk, spiral arms, or ongoing major mergers. Some minor asymmetry may be present, suggesting a possible past interaction. Overall, the galaxy presents as a relatively quiescent system with moderate luminosity and estimated mass.
