This galaxy presents as a relatively smooth, centrally concentrated object with a predominantly elliptical morphology. There is a high degree of central light concentration, with the galaxy appearing nearly spheroidal, and the isophotes are generally regular. There is a minimal indication of spiral arm structures or other significant disk features. It exhibits a color gradient, with the central region appearing more yellow-red, suggesting an older stellar population, while the outer regions appear slightly bluer, indicating the presence of some younger stars. There is no strong evidence of significant tidal distortions, major mergers, or strong bar structures. There might be a faint hint of a minor disturbance in the overall structure, but more data is needed to verify. The overall impression is that of a fairly evolved, passively evolving system.
