  We present high spatial resolution, near-IR images in J, H, K of the nucleus
of NGC3227, obtained with the Adaptive Optics bonnette on CFHT. The ~0.15
arcsec (17pc) resolution allows structures to be probed in the core region.
Dust obscuration becomes significantly less pronounced at longer wavelengths,
revealing the true geometry of the core region. We are able to identify two
main features in our maps: (i) a spiraling association of knots with a
counterpart in an HST F606W image; (ii) a smaller scale annulus, orthogonal to
the spiral of knots. These features may provide a means to transport material
inwards to fuel the active nucleus.
