The galaxy presents as a spiral type, observed at a moderate redshift. It exhibits a prominent disk structure. The spiral arms are readily apparent, displaying a generally open winding pattern. Two main spiral arms are visible. The arms are well-defined with a clumpy morphology, suggesting active star formation regions. A bar structure seems to be present, with a moderate prominence crossing the galactic center. The central bulge appears relatively small. There are potential signs of tidal disturbances or minor merger activity, though the overall structure remains largely intact. The color indices suggest a relatively blue population, which indicates the presence of young, hot stars in the spiral arms.
