The galaxy presents as a relatively compact, elliptical object with a smooth light distribution. The primary color is a yellowish-white, suggesting a population of older stars. There is a distinct, redder, and more compact core slightly offset from the main body. This may indicate an Active Galactic Nucleus or a region of intense star formation heavily obscured by dust. There is no evidence of spiral arms or a distinct disk component. The overall form suggests a system that has undergone significant dynamical evolution. There is no obvious major ongoing merger event but there may be tidal features that are too faint to resolve from this image, potentially indicating a past interaction.
