The galaxy appears as a centrally concentrated, smooth object. There is a lack of discernible spiral arms or significant disk structures. The galaxy exhibits a nearly circular morphology. Color gradients suggest a radial variation in stellar populations, with a yellowish core potentially indicative of older stars and/or dust obscuration, transitioning to slightly bluer hues in the outer regions, potentially indicating more recent star formation. There are no signs of major disturbances or ongoing mergers visible in the image.
