The galaxy presents as an elliptical morphology with a smooth, featureless appearance. It displays a concentrated central bulge, and minimal visible structure within the diffuse halo. The color profile suggests a population of older stars, with a dominant yellow-red hue indicative of a relatively low rate of current star formation. The overall form of the galaxy suggests it is relatively undisturbed, without any obvious tidal tails, shells, or other signs of recent major mergers or interactions. It is a relatively massive system.
