This galaxy appears to be a relatively smooth and rounded elliptical galaxy. There is a concentrated central bulge that gradually fades into a more diffuse halo. It exhibits a yellowish-white color, indicating a likely population of older stars. There is no discernible disk structure or spiral arms visible. The overall morphology suggests a galaxy that has undergone significant evolution and is likely quiescent in terms of current star formation activity. There's some indication of minor disturbances within the galaxy.
