The galaxy appears as a flattened spheroid, suggesting it is likely an elliptical galaxy viewed at an oblique angle. The galaxy exhibits a smooth, centrally concentrated light profile, with the highest intensity appearing towards the core. The light smoothly diminishes outward from the center. There is a subtle color gradient, where the central region appears slightly more yellow/orange, which indicates an older stellar population. The outer regions appear slightly bluer. Based on the observed morphology, there is no distinct evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no obvious signs of recent mergers or major interactions.
