The observed galaxy appears to be a spiral galaxy at an appreciable distance, evident from its redshift. The galaxy presents a distinct central bulge with an apparent yellow hue, suggesting an older stellar population dominating the core. Fainter spiral arms are visible extending from the central bulge, exhibiting a bluer color, indicating ongoing star formation. The morphology suggests a relatively low star formation rate, with a high mass. There is a lack of major mergers or disturbances present in this image.
