The galaxy presents as a relatively smooth, elliptical structure. It exhibits a bright, concentrated central bulge, indicating a high stellar density in the galactic nucleus. The light distribution appears to gradually diminish from the core outward. There is a slight elongation of the galaxy's shape, with the major axis extending horizontally in the image. The overall color appears yellowish-white, suggesting a population of older stars. No distinct spiral arms or dust lanes are discernible, supporting its classification as an elliptical galaxy. There is a very slight hint of possible merging activity and minor disturbances, but they are barely noticeable.