The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that fades into a more diffuse halo. The light distribution is generally even, with a slight elongation suggesting it is not perfectly spherical. There is a subtle color gradient from the core outwards, with the central region appearing slightly redder. No distinct dust lanes or spiral arms are observed. The galaxy shows no obvious signs of major disturbances or ongoing merger activity. 
