The galaxy exhibits a distinct spiral structure, with tightly wound arms emanating from a prominent central bulge. The bulge appears moderately sized in relation to the overall galactic disk. The spiral arms display a clumpy texture, suggesting regions of active star formation. The overall color of the disk leans towards blue, indicative of a relatively young stellar population. A bar structure appears to be present extending across the bulge. There is no apparent sign of any major merging events.
