The galaxy presents a spiral morphology with a central bulge of moderate size. Two distinct spiral arms appear to dominate the disk structure, exhibiting a winding pattern ranging from medium to somewhat loose. A weak bar structure may be present, though this is not definitively discernible in the available imagery. There is no indication of significant merger activity or major disturbances. The disk shows clumpy regions of star formation activity. Overall, it looks like a fairly normal spiral galaxy, with some evidence of an active star-forming region within its disk.
