The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The light distribution appears elliptical, with a moderate axis ratio, indicating a somewhat flattened shape. There is no evidence of spiral arms or a prominent disk structure. The galaxy exhibits a color gradient, transitioning from a yellowish-white hue in the central region to a redder tint in the outer parts, which could indicate an older stellar population in the outskirts. There might be signs of minor disturbances nearby, but it's difficult to tell without additional information.
