The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a color gradient, appearing yellowish-white in the core and gradually transitioning to a slightly bluer hue toward the outer regions. There is no discernible spiral arm structure or significant dust lane obscuration evident in this image. The overall morphology suggests a well-mixed stellar population, and there is no indication of ongoing major mergers or significant tidal disturbances in this image.
