The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the center, there's a gradual decrease in luminosity, with the color transitioning to a slightly redder tone. No distinct spiral arm structures are visible. The overall shape is round, with no apparent distortions indicating any recent or ongoing major mergers. Minor disturbances cannot be ruled out. The galaxy has a relatively compact size. The light distribution suggests it is likely an early-type galaxy, potentially an elliptical or lenticular galaxy with little to no ongoing star formation.
