The galaxy appears to be a relatively bright, centrally concentrated system. It presents a largely smooth and rounded morphology, with no immediately apparent spiral arm structure or significant disk features visible in this imaging. The light profile suggests a fairly well-defined central bulge, surrounded by a more diffuse halo of stars. There may be some subtle color gradients, with the central region appearing more yellow/gold tinged, potentially indicating an older stellar population, while the outer regions exhibit bluer hues, possibly suggesting some on going, albeit low, star formation. There is no obvious evidence of tidal interactions or major merger events influencing its current structure.
