The galaxy presents as a centrally concentrated object with an ellipsoidal morphology. The core exhibits a bright, compact region, possibly indicative of an active galactic nucleus or a dense stellar population. A faint, extended halo surrounds the core, with the suggestion of a disklike component. There is an indication of some internal structure within the core region, but details are difficult to resolve. Overall, the galaxy appears relatively undisturbed, without strong signs of a recent major merger, though there are some indications of possible minor disturbances. The color gradient suggests a gradient in stellar populations, dust content, or both, from the center outwards, with the central regions appearing bluer and the outer regions exhibiting redder hues.
