The galaxy presents as a relatively compact object. Its morphology appears predominantly smooth and round, with no obvious spiral arms or bar structures visible. The galaxy exhibits a color gradient, with the central region appearing slightly more yellow or golden, transitioning to a bluer hue in the outer regions. This color variation may indicate differing stellar populations and ongoing star formation in the outer disk. Based on its redshift, the galaxy is relatively distant, and thus appears faint in the image. No significant signs of recent or ongoing major mergers are apparent, though minor disturbances or interactions cannot be ruled out.