The galaxy exhibits a distinct spiral structure. Two prominent spiral arms are clearly visible, winding moderately around a central bulge. The winding of the spiral arms appears neither tightly wound nor exceptionally loose. The bulge presents a moderate size relative to the overall galactic disk. The galactic disk shows a relatively flat orientation. The central bulge is characterized by a yellow-orange hue, indicative of an older stellar population. Star formation appears active, with blue-ish tones and a hazy appearance within the spiral arms, suggestive of regions of ionized gas and young, massive stars. There is no evident bar structure spanning the bulge. Overall, the disk displays a fairly undisturbed structure, though some minor distortion could be occurring. There are no clear indications of major mergers, or any substantial interactions.
