The galaxy presents a defined spiral structure. Its morphology suggests a disk-dominated system, with tightly wound spiral arms emanating from a central bulge. The bulge appears relatively small in comparison to the overall disk size. The spiral arms show a complex, multi-armed structure, though precise arm count is difficult to discern due to resolution limitations. There is no clear indication of a prominent bar feature. No signs of a major merger event is observed, though some minor disturbances may exist. The galaxy appears relatively undisturbed.
