The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated, centrally bright core that fades gradually into its outer regions. There is a slight elongation noticeable in the galaxy's shape, indicating that it is not perfectly spherical, but is more of a flattened or disc-like structure viewed at an angle. The color gradient suggests a population of older stars, giving off the yellowish-orange hue, particularly in the core, implying less ongoing star formation. There might be some slight disturbances visible as subtle color variations, but overall, it seems to be a fairly undisturbed system.
