The galaxy presents as a somewhat elliptical, relatively smooth, and centrally concentrated object. The light profile suggests a spheroid-dominated system with little discernible disk component or spiral arm structure. There is a color gradient, with the central region appearing more yellow, shifting toward red at the outer edges. This may be due to a difference in stellar populations, with older, redder stars dominating the outer regions, and younger, bluer stars in the center. There are no clear signs of major merger activity, although minor tidal disturbances cannot be ruled out due to the limited resolution. The overall appearance suggests a mature galaxy with ongoing, but relatively low, star formation.
