The galaxy appears as a somewhat diffuse, elliptical object with a slightly brighter central region. The overall color is a pale blue-white, suggesting the presence of younger stars, particularly within the central bulge. There is a subtle gradient in brightness from the center outwards, indicating a decreasing stellar density towards the edges of the galaxy. The galaxy seems relatively undisturbed, lacking any obvious signs of spiral arms or tidal features indicative of a recent merger or interaction. The light distribution implies a relatively smooth stellar population throughout the galaxy.
