The galaxy presents as a smooth, single concentration of light. The morphology appears largely undisturbed, with no obvious signs of tidal tails, bridges, or other indicators of recent major mergers or interactions. The shape of the galaxy is neither perfectly spherical, nor extremely elongated, tending towards a more oblate form. It seems to have an elliptical-like morphology, with no readily apparent spiral arm structure, and a significant, central bulge. The galaxy presents a dominant yellowish hue, which implies a population of older stars and a relatively low rate of on-going star formation.
