  We have been monitoring the binary system V0332+53 (optical counterpart is BQ
Cam) since 2004 using 45 cm ROTSEIIId telescope and RTT150 (Russian-Turkish 1.5
m Telescope) located at Bakirlitepe, Antalya, Turkey. We report on the
long-term variability of this system up to the present date. There exists a
fading of 0.2 mag in the light of BQ Cam after MJD 53400. The fading in the
light curve of BQ Cam could be due to a decrease in the density or in the size
of the circumstellar disk.
  We present optical spectroscopic observations obtained before (at MJD 54730)
and during (at MJD 54768) the new X-ray activity reported by Krimm et al.
(2008). The observed Ha line profiles were single-peaked and almost symmetric.
The present EW values are found to be similar to the ones observed during the
fading of infrared magnitudes of Negueruela et al. (1999). Ha emission lines
were found to be red-shifted by ~140 km/s which were larger than the findings
of Corbet et al. (1986). We suggest that brightening of the disk after MJD
54700 may be due to the precession of the disk.
