The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse light distribution. There is a slight elongation visible, although the overall shape is predominantly round. The central region exhibits a bright, concentrated core that fades gradually outwards. The color is generally yellow-white, suggesting an older stellar population, though there is some hint of bluer components. No distinct spiral arms or prominent dust lanes are discernible. The galaxy appears relatively undisturbed, without major morphological distortions or signs of ongoing merger activity.
