The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse appearance. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the center, the light gradually fades. There is some subtle reddening on the left side of the galaxy. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears relatively isolated, showing no obvious signs of major tidal disruption or interaction with other galaxies in its immediate vicinity.
