The galaxy presents as a singular, elliptical-like structure with a smooth, concentrated central region. The central region is significantly brighter than the surrounding area, with a yellow-white hue suggesting an older stellar population. There are no obvious spiral arms or significant dust lanes visible. The overall color gradient transitions from a yellow-white core to a slightly redder outer halo. The edges appear diffuse. There is no evidence of any major ongoing merger events. The galaxy is relatively round in shape.
