The galaxy presents as a centrally concentrated, smooth, elliptical-like morphology. The light profile appears highly regular, lacking any prominent spiral arm structures or significant dust lane obscuration. The core region is intensely bright, decreasing radially into a more diffuse halo. The overall color is yellowish-orange, hinting at an older stellar population. It exhibits an apparent lack of any major tidal disturbances or signs of recent merger activity, although there may be a very slight asymmetry in the outer halo. The galaxy's roundness suggests that it does not exhibit a significant disk component, rather it may be spheroidal in nature.
