The galaxy presents as a face-on spiral, exhibiting a defined disk structure. The spiral arms are prominent and traced by areas that suggest active star formation regions. The galaxy appears flocculent, indicating that the spiral arms are not well-defined and continuous, but rather patchy. A weak central bar is suspected, with a moderate bulge component. The galaxy appears to be relatively isolated, with no clear signs of major interaction or merging events. The morphology indicates a well-defined structure, but with some level of disturbance visible in the outer arms.
