  We present an analysis of archival Gemini g', r', K and Keck H, K_s imaging
of this nearby short period binary (P_B=95.8min) 2.87ms pulsar. The heated
companion is clearly detected. Direct pulsar heating provides an acceptable
model at the revised >700pc parallax distance. The relatively shallow light
curve modulation prefers an inclination i<40deg; this high latitude view
provides a likely explanation for the lack of radio signatures of wind
dispersion or eclipse. It also explains the low minimum companion mass and,
possibly, the faintness of the source in X- and gamma-rays.
