The galaxy appears to be elliptical in morphology. The light profile suggests a centrally concentrated bulge component, with a smooth, diffuse halo extending outwards. The galaxy exhibits a color gradient, with the central region appearing more yellow/orange, potentially indicating an older stellar population, while the outer regions appear slightly bluer. There is no discernible spiral arm structure or dust lanes visible in the image, reinforcing the classification of an elliptical galaxy. The overall light distribution is relatively uniform and symmetrical. There are no signs of major tidal disturbances or interactions with other galaxies.
