  A new two-image gravitational lens system has been discovered as a result of
the Cosmic Lens All-Sky Survey (CLASS). Radio observations with the VLA, MERLIN
and the VLBA at increasingly higher resolutions all show two components with a
flux density ratio of ~7:1 and a separation of 1.34". Both components are
compact and have the same spectral index. Followup observations made with the
VLA at 8.4 GHz show evidence of a feature to the south-east of the brighter
component and a corresponding extension of the weaker component to the
north-west. Optical observations with the WHT show ~1.7" extended emission
aligned in approximately the same direction as the separation between the radio
components with an R-band magnitude of 21.8 +/- 0.4.
