The galaxy exhibits a distinct spiral morphology, characterized by prominent spiral arms. These arms appear loosely wound, extending outwards from the galactic center. A bar-like structure is present, with a moderate strength, traversing the galaxy's core. The bulge appears small relative to the overall size of the galaxy, with no dominant features. There are two spiral arms. There is no major merging events, but some minor disturbances. The galaxy exhibits a color profile consistent with ongoing star formation, with bluer regions concentrated within the spiral arms, suggestive of younger stellar populations. Overall, the galaxy displays features characteristic of a spiral galaxy with active star formation and a relatively undisturbed structure.