We present the results of broad band polarimetry, spectropolarimetry,
and spectrophotometry of the narrow-line, IR-Ultraluminous galaxy IRAS
09104+4109 (L = 6 x 10(12) L. h-2, z = 0.442). We conclude that this
cD galaxy hides a luminous quasar that powers the infrared emission (a
possibility first suggested by Kleinmann et al. 1988) - a hole in the
dust allows the quasar light to escape, ionizing the extended narrow
line region. Some of the emerging quasar light is seen as highly-polar
ized (scattered) ultraviolet continuum and a broad MgII emission line.