The galaxy presents as a grand design spiral, with a well-defined disk structure and prominent spiral arms. The arms exhibit a tightly wound morphology, emanating from a distinct, bright central bulge. Within the spiral arms, there are several regions displaying enhanced blue luminosity, suggestive of active star formation. The bulge appears relatively small in comparison to the overall disk size, suggesting a less dominant bulge component. There is no clear indication of a bar structure bisecting the bulge. The spiral arms are somewhat patchy in appearance, exhibiting variations in luminosity and color. The galaxy's disk appears relatively undisturbed, without significant signs of tidal interactions or major merger events, though some minor disturbances may be present. Overall, the galaxy appears to be a relatively isolated spiral system, undergoing active star formation within its spiral arms.
