The galaxy presents as a flattened, elliptical morphology. The central region exhibits a high concentration of light, appearing smooth and generally featureless. The color gradient suggests a population of older stars concentrated towards the center. The outer regions appear less luminous, extending into a somewhat elongated shape. There is a subtle hint of disk-like structure. No signs of major mergers or significant tidal disturbances are apparent in this image. The overall appearance indicates a mature system, potentially undergoing low levels of star formation activity.
