This galaxy presents a primarily smooth and rounded morphology, with a color profile that shifts from a warm, yellowish-orange core to cooler, greenish-yellow edges. The central region exhibits a high degree of concentration, suggesting an older stellar population. There may be a disk or spiral structure, but it is not clear from the image, as it is largely blended into the main body of the galaxy. There is no sign of any major ongoing merger activity, but there may be slight disturbances on the edges of the galaxy. Based on the colors, the galaxy has likely undergone minimal star formation.
