  HE 0141-3932 (zem = 1.80) is a bright blue radio-quite quasar with an
unusually weak Ly-alpha emission line. Large redshift differences (Delta z =
0.05) are observed between high ionization and low ionization emission lines.
Absorption systems identified at zabs = 1.78, 1.71, and 1.68 show mild
oversolar metallicities (Z ~= 1-2Zsolar) and can be attributed to the
associated gas clouds ejected from the circumnuclear region. The joint analysis
of the emission and absorption lines leads to the conclusion that this quasar
is seen almost pole-on. Its apparent luminosity may be Doppler boosted by ~10
times. The absorbing gas shows a high abundance of Fe, Mg and Al ([Fe, Mg,
Al/C] ~= 0.15 +/- 0.10) along with underabundance of N ([N/C] <= -0.5). This
abundance pattern is at variance with current chemical evolution models of QSOs
predicting [N/C] >= 0$ and [Fe/C] < 0 at Z ~ Zsolar.
