The galaxy presents a disk-like structure with clear spiral arm morphology. These arms are well-defined and exhibit a relatively open winding. Dust lanes are visible within the spiral arms, contributing to the overall patchy appearance. A central bulge is apparent, displaying a moderate size relative to the disk. There is no clear evidence of a strong bar structure. The galaxy appears to be undergoing significant star formation, indicated by the presence of bright knots or clumps within the spiral arms. These likely represent regions of active starbirth. There is no substantial evidence of ongoing major merger activity, although minor disturbances may be present based on some asymmetry in the outer disk region. Overall, the galaxy appears to be a relatively undisturbed spiral galaxy with ongoing star formation.
