The galaxy exhibits a prominent disk structure, characterized by well-defined spiral arms. The arms display a tightly wound morphology, suggesting a higher shear rate within the disk. There appears to be no strong central bar feature. The bulge component is relatively small, implying that a significant portion of the galaxy's light is dominated by the disk. Within the spiral arms, areas of ongoing star formation are evident, visible as brighter, bluer regions. There appears to be no evidence of major mergers or significant tidal distortions in the galaxy's morphology. The galaxy displays a moderate inclination, allowing for clear observation of the spiral arm structure. Overall, the galaxy presents as a relatively undisturbed spiral galaxy with active star formation within its disk.
