The galaxy appears as a relatively smooth, centrally concentrated object. Its overall shape is somewhat elliptical. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars and potentially a supermassive black hole actively accreting material, though no distinct active galactic nucleus is readily apparent in this image. The outer regions of the galaxy fade gradually, with a subtle decrease in surface brightness. There is no discernible spiral structure or pronounced disk component.
