This galaxy appears to be a spiral type, exhibiting a disk structure. The disk presents with moderately wound spiral arms, suggesting an intermediate morphology between grand design and flocculent. The spiral arms are somewhat tightly wound. The image shows what appears to be two distinct spiral arms. A bar structure is possibly present across the galaxy's bulge, appearing to be weak. The bulge is moderate in size compared to the disk. There is no evidence of a major merger, though the galaxy does show some possible disturbances or signs of interactions, such as a faint tail of light extending from one side of the galactic disk. The disk is oriented face-on. The galaxy exhibits a blue color suggesting ongoing star formation.
