The galaxy presents as a spiral type, exhibiting well-defined spiral arms originating from a central bulge. The arms appear to be grand design, with a clear, organized structure winding outwards. There is evidence of active star formation within these arms, indicated by the clumpy, knotty texture and subtle blue hues.

The central bulge is prominent, and it displays a smooth, yellowish-white color gradient, suggesting an older stellar population. The disk appears to be viewed at a moderate inclination, allowing for a good view of both the spiral structure and the bulge. The galaxy exhibits a slight asymmetry, with one spiral arm being more tightly wound than the other, possibly due to tidal interactions or internal dynamics. Overall, this galaxy appears to be a relatively massive, actively star-forming spiral with a well-defined structure and a prominent central bulge.
