The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core region exhibits a bright, yellowish-white hue, indicating a potential population of older stars or significant dust obscuration. Progressing outwards from the center, the galaxy displays a gradual decline in surface brightness and a transition in color. Subtle color gradients are present, transitioning toward a redder hue in the outer regions which suggests older stellar populations present in this region. There are potentially some faint features that may be part of a disturbed morphology, or possibly artifacts, but these are very difficult to definitively conclude based on the image alone. Overall, the galaxy appears relatively undisturbed and potentially contains little to no ongoing star formation.
