This galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, with a diffuse halo extending outwards. The overall color profile suggests a redder, more evolved stellar population, consistent with a low star-formation rate. While the galaxy appears mostly undisturbed, there might be subtle signs of minor interaction or internal activity. There is no clear presence of prominent spiral arms or dust lanes visible in this image. The general roundness of the galaxy is evident.
