The observed galaxy presents as a relatively compact spiral galaxy with a redshift indicating it is at a considerable distance. The galaxy exhibits a defined, though not particularly prominent, central bulge. The spiral arms appear tightly wound and are host to some star forming regions which are visible as subtle colour variations. A bar structure may be present, but it is subtle and difficult to discern clearly from the current observational data. The overall morphology suggests a galaxy undergoing active star formation with a mass that would categorize it as a relatively average spiral galaxy. There is no clear indication of ongoing major merger activity, though minor disturbances may be present in the outer disc. The galaxy's light distribution indicates the presence of both older stellar populations in the central bulge and younger, bluer stars within the spiral arms. The galaxy is roughly estimated to be about 9 kpc wide.
