The galaxy presents as a spiral type, with discernible arm structures emanating from a subtle central bulge. These spiral arms exhibit a somewhat flocculent morphology. There appears to be evidence of ongoing star formation activity within the arms, as suggested by the presence of bluer regions. Dust lanes are subtly visible within the disk, obscuring some of the starlight. Overall, the galaxy exhibits a face-on orientation relative to our line of sight. There is an apparent companion galaxy to one side. It is unclear whether the morphology of either is distorted.
