The object appears to be a spiral galaxy, observed at a redshift that indicates it is at a considerable distance. It displays a disk-like structure with a distinct central bulge. The bulge appears moderately sized and exhibits a yellowish hue, potentially indicating an older stellar population. Two well-defined spiral arms emanate from the central region, displaying a winding pattern best described as medium in tightness. Star formation is observed within these arms, signified by the presence of bluer regions. The overall morphology suggests a relatively quiescent state, with no apparent signs of major mergers or significant tidal disturbances. There might be a faint indication of a bar structure.
