  We report the discovery of optical and X-ray synchrotron emission from the
brighter radio jet in galaxy NGC 7385 using data from HST and Chandra. The jet
has a projected length of 5 kpc and a similar morphology to other known optical
jets in low-power radio galaxies. We also report a strong jet-cloud interaction
which appears to be deflecting the counter-jet and causing a reversal in its
direction.
