We interpret the data on the nearby active galaxy IC 5063 (PKS 2048-57
) within the framework of an obscured quasar, as proposed by current u
nified schemes for active galactic nuclei (AGN). We apply new techniqu
es to estimate the reddening towards the nucleus of obscured AGN, base
d on infrared photometry and line-to-continuum correlations, and concl
ude that the previously claimed detections of the transmitted quasar c
ontinuum in the H and K bands are probably due to the presence of fore
ground dust, which results in reddening of the starlight within small
apertures. From the data available on this object and established corr
elations between quasar properties, we deduce the amount of visual obs
curation towards the active nucleus in IC 5063 to be in the range A(V)
= 65-105 mag.