The galaxy presents as an elliptical system. It exhibits a generally smooth and concentrated morphology with no discernible spiral arms or bar structures visible. The galaxy appears largely spheroidal, though there is a slight elongation. The core region exhibits a bright, yellow-shifted luminosity, suggesting a population of older stars. The outer regions of the galaxy fade gradually into the background, forming a diffuse halo. The image reveals no signs of recent or ongoing major mergers or significant tidal disturbances. Overall, the galaxy appears to be relatively undisturbed and evolved.
