The galaxy presents a disk-like structure with prominent spiral arms. The arms are relatively tightly wound, exhibiting a flocculent structure, appearing somewhat fragmented and less defined in certain regions. The central bulge is moderately sized, with a yellowish-white hue, suggesting an older stellar population. The disk shows a bluer color, indicating ongoing star formation. There is no obvious bar structure visible. There are no signs of major merging events, but it is possible that the galaxy may have experienced or be currently experiencing a minor interaction based on the slight asymmetries in the outer disk. The spiral arms have an estimated average of 2 arms.
