The galaxy presents as a luminous object with a relatively smooth, rounded morphology. There is an indication of a double nuclei in the image, this could be evidence of a galactic merger or a recent interaction with another galaxy. Color gradients suggest a complex stellar population, with a central region appearing more concentrated and potentially older, as indicated by the yellowish hue. The outer regions display a bluer tone, possibly indicative of younger stars and ongoing star formation. Overall, the galaxy appears to be relatively massive and actively evolving, with potential signs of past or ongoing mergers influencing its structure and stellar content.