The galaxy appears as a single, moderately bright object with a smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core. The overall color appears somewhat red, suggesting an older stellar population and/or significant dust obscuration. There may be a hint of a diffuse, extended halo or envelope surrounding the central region, but the faintness and blurry image quality make it difficult to discern any detailed structure. No obvious spiral arms or strong dust lanes are visible. The galaxy seems relatively undisturbed, without any apparent signs of a major ongoing merger or tidal disruption.
