This galaxy presents an elliptical morphology. It exhibits a smooth, centrally concentrated light distribution, with a gradual decline in surface brightness outward from the core. The core region appears yellowish, indicating a population of older stars. Moving outward from the center, the galaxy displays a bluer hue, suggesting a component of younger stars. There is no discernible dust lane or spiral arm structure. The galaxy appears relatively undisturbed, lacking any obvious signs of recent major merger activity, though minor disturbances cannot be ruled out. Overall, the galaxy appears to be an evolved system with ongoing, low levels of star formation. The shape is more elongated than circular.
