Near-infrared imaging with the Hubble Space Telescope recently revealed a circumstellar dust disk around the A star HD 32297 .
Dust scattered light is detected as far as 400 AU radius and the linear morphology is consistent with a disk \sim 10 \arcdeg away from an edge-on orientation .
Here we present the first optical images that show the dust scattered light morphology from 560 to 1680 AU radius .
The position angle of the putative disk midplane diverges by \sim 31 \arcdeg and the color of dust scattering is most likely blue .
We associate HD 32297 with a wall of interstellar gas and the enigmatic region south of the Taurus molecular cloud .
We propose that the extreme asymmetries and blue disk color originate from a collision with a clump of interstellar material as HD 32297 moves southward , and discuss evidence consistent with an age of 30 Myr or younger .