Maps of the Fe ii* emission from the blue-shifted (left) and redshifted (right) outflow components with 2 × 2 Gaussian smoothing. The black lines show the two slit positions at +70°, and −20°. The white crosses indicate the galaxy major and minor axes from the Contini et al. (2016) kinematic analysis of [O ii]. The strongest emission from both the red and the blue-shifted components is roughly spatially coincident. In the case of a bi-conical outflow, this suggests that we may be observing emission predominantly from the base of the wind, not far from the plane of the galaxy.