The galaxy appears to be a spiral galaxy, observed at a redshift of approximately 0.11. It presents a disk structure, though not perfectly edge-on, with a relatively compact bulge. The spiral arms are well-defined, displaying a winding pattern, predominantly featuring two arms. These arms show evidence of active star formation regions, inferred from their bluer hue. There is no strong evidence of a bar structure at the center. The bulge appears yellowish and smaller relative to the disk. No major signs of ongoing merging or significant tidal disturbances are immediately apparent. The overall morphology suggests a spiral galaxy with moderate to strong star formation activity within its spiral arms.
