The galaxy presents as a relatively smooth, elliptical structure. It exhibits a prominent central bulge that gradually diffuses into the outer regions, displaying a centrally concentrated light profile. The galaxy is not perfectly circular, showing a slight elongation along a major axis. The color gradient suggests an older stellar population, with the central bulge appearing more yellow/orange and the outer regions slightly bluer, potentially indicating regions of more recent, albeit diminished, star formation. There is no apparent indication of spiral arms, bar structures, or active galactic nuclei based on the morphology presented in the image. The galaxy does not seem to be heavily disturbed or undergoing a major merger event.
