  We report on Chandra imaging observations of the Galactic Unidentified
$\gamma$-ray source GEV J1809-2327, comparing the X-ray images with new VLA
1.46 GHz and 4.86 GHz maps. The X-ray images reveal a point source connected to
a non-thermal X-ray/radio nebula, supporting a pulsar/wind model for the
$\gamma$-ray emitter. We also detect numerous X-ray sources from the young
stellar association in the adjacent HII region S32.
