The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated core. It exhibits a radial gradient in brightness, with the intensity decreasing steadily from the core outwards. The galaxy displays an overall yellowish-orange hue, suggesting a population of older stars. A faint, diffuse halo surrounds the central region, indicating a more extended stellar distribution. There's a subtle elongation observed, with the galaxy deviating slightly from a perfectly circular shape, possibly indicating it's a disk galaxy viewed at an angle. No distinct spiral arms or prominent dust lanes are discernible. Minor asymmetrical features are observed, which could indicate a history of minor galactic interactions.
