The optical and radio spectrum as well as direct imaging data for the
strong radio source S4 1745 + 624, a high redshift quasar with z = 3.8
86, are presented. The optical continuum redward of Lyman alpha is rat
her steep with a spectral index of alpha = - 1.3 and the continuum dep
ression blueward of the Lyman alpha lambda1216 emission line is smalle
r than in optically selected quasars of similar redshift. The overall
radio spectrum differs markedly from that of other high redshift radio
quasars, showing a steep low frequency part and a flat high frequency
part.