The galaxy appears as a centrally concentrated, elliptical-like structure. The core region exhibits a bright, yellowish hue, indicating a population of older stars. The galaxy appears to be smoothly structured, with no obvious spiral arms or distinct features. The outer regions of the galaxy fade in intensity, suggesting a gradual decrease in stellar density away from the core. The overall shape indicates a degree of elongation, not quite circular. There are no clear signs of active merging or major disturbances, although subtle asymmetries may be present.
