The galaxy appears to be a spiral galaxy, observed at a redshift of approximately 0.27. It exhibits a prominent disk structure with evidence of spiral arms. These arms display a range of winding tightness from tight to loose, with at least two prominent arms visible. There is some visual indication of ongoing star formation within the arms. The central bulge of the galaxy appears relatively compact and of moderate size. The galaxy shows no obvious signs of being an edge-on disk galaxy, and there may be some minor gravitational disturbances or interactions. The presence of a bar structure is not definitively discernible but is weakly suggested. There may be two main spiral arms.