The galaxy exhibits a prominent disk structure, tilted relative to our line of sight. This disk displays distinct spiral arm morphology. These arms appear relatively tightly wound in some areas and loosely wound in others, tracing a two-armed spiral pattern. The central bulge region is moderately sized, exhibiting a yellowish hue, suggestive of an older stellar population. A bar feature appears to extend across the central region of the galaxy, though not particularly strong. Some areas of the disk show localized brighter regions, likely indicative of star-forming regions. There is no apparent major disturbance or significant merging activity evident in the galaxy's morphology, although there could be a minor disturbance within the galaxy.
