3C 133; z=0.277

We have discovered a new optical-IR jet in 3C 133 See [Floyd et al.2006] for further discussion. The jet and eastern hotspot are well resolved, and visible at both optical and IR wavelengths, in spite of the low galactic latitude. The infrared jet follows the morphology of the inner part of the radio jet, with three distinct, aligned, bright knots east of the unresolved nucleus. The host is a round elliptical.