The galaxy presents as a flattened elliptical structure, approximately two-thirds as wide as it is long. Its central region appears quite bright and concentrated, suggesting a significant stellar population density in the core. The light distribution exhibits a smooth gradient, diminishing outwards from the nucleus, indicating an evenly distributed stellar population. There is a slight bluing of the color in its outer edges. Overall, the galaxy appears relatively undisturbed with no obvious signs of tidal interactions or major morphological distortions.
