The observed galaxy presents a morphology consistent with a spiral galaxy, exhibiting a disk-like structure. Two prominent spiral arms appear to emanate from a central bulge, indicating a grand design spiral structure. These arms are not tightly wound. The galaxy is not edge-on but rather slightly inclined, which allows for a partial view of the spiral arms. The bulge appears moderately sized compared to the overall size of the galaxy. The bar structure looks present and prominent. There appear to be regions of active star formation, as indicated by the observed color. There is no obvious strong evidence of a major merger in the images, however, I do see what could be described as minor disturbances.
