The galaxy appears to be a relatively compact and smooth system. It exhibits a centrally concentrated brightness profile, with luminosity decreasing radially outward. There is no strong evidence of spiral arm structure or a prominent disk, suggesting a classification as an elliptical or lenticular galaxy. The overall color is somewhat neutral, with a slight green hue. The lack of significant blue light indicates a paucity of young, massive stars, implying a relatively low current star formation rate. There does not appear to be any evidence of major ongoing mergers or significant tidal disturbances. Faint outer regions appear symmetrical and undisturbed. The overall morphology suggests a galaxy that has largely ceased active star formation and has evolved towards a more quiescent state.
