  We demonstrate through the use of a simple toy model that asphericity in dark
matter halos has a measurable effect on the configuration dependence of the
weak lensing shear 3-point function at small scales. This sensitivity provides
a way, in principle, to measure the shapes of dark matter halos. The
distribution of halo ellipticities should be included in models aiming at a
high fidelity prediction of n-point shear correlation statistics.
