The galaxy displays a clear disk structure with noticeable spiral arm features. The arms appear relatively tightly wound, suggesting an intermediate spiral type. There is evidence of flocculent structure along the spiral arms, with areas of active star formation. The central bulge is prominent and moderately sized, with a yellowish hue indicating an older stellar population. No obvious bar structure is visible in this image. The galaxy's light profile indicates a fairly smooth transition from the bulge to the disk. There are no obvious signs of a major merger event, although minor disturbances or interactions can't be ruled out based on the morphology alone. The overall color suggests a mix of stellar populations with ongoing star formation activity. The galaxy appears to be neither perfectly edge-on nor face-on, allowing for a detailed examination of its spiral structure.
