The galaxy presents as a slightly elongated elliptical form. It exhibits a smooth, centrally concentrated light distribution, with the brightest region located at the core. The galaxy appears to have a shallow brightness gradient, gradually fading into the background sky. The core region is noticeably more luminous than the surrounding areas, suggesting a high stellar density. The overall color of the galaxy is relatively uniform, with a slightly redder hue than would be expected from a pure spiral disk. The galaxy shows no evidence of prominent spiral arms or dust lanes. The edges of the galaxy are somewhat diffuse, lacking a sharp or well-defined boundary. There are a few hints of some star forming regions, but there isn't much active star formation occurring.
