The object appears to be a spiral galaxy, observed at a redshift indicating a considerable distance. The galaxy exhibits a disk-like structure, with prominent spiral arms extending outwards from a central bulge. The arms are well-defined and loosely wound. The spiral structure suggests active star formation. The central bulge is relatively moderate in size. There is no apparent strong bar structure bisecting the bulge. No signs of ongoing major mergers were observed, although minor disturbances may be present in the morphology.
