The galaxy presents as a relatively smooth and concentrated object, with an elliptical morphology. The light distribution suggests a dominant bulge component, with the highest intensity concentrated towards the center. A fainter, more diffuse halo extends outwards from the core. The color is generally redder in the central regions, possibly indicating an older stellar population, with the outer regions showing a slightly bluer hue. No distinct spiral arms or prominent dust lanes are apparent in the image. The overall impression is that of a relatively quiescent galaxy.
