The object presents as a spiral galaxy exhibiting a notable disk structure. The galaxy displays two prominent spiral arms that appear well-defined, exhibiting a medium to loose winding pattern. The central bulge appears small relative to the disk, suggesting a late-type spiral morphology. A weak bar-like structure seems to be present traversing the central region. The galaxy does not display any obvious signs of major interaction or merging events. The spiral arms show clumpy regions of star formation. The galaxy exhibits a redshift, indicating it is at a cosmological distance.
