Near Infrared Camera and Multi-Object Spectrometer (NICMOS) H-band image (top) of the lensing system from Kochanek et al. (1999), and the Stokes I (middle) and polarized intensity (PI, bottom) maps from our VLA data. A and B indicate the lensed images of the background quasar, and G shows the lensing galaxy. The lensing galaxy can only be seen in the NICMOS H image, and is too faint to be detected in our VLA images. The Stokes I and PI maps are 16 MHz channel maps at 3.7 GHz. The beam size is shown in the lower left corner.