  We present multi-colour CCD photometry of GSC4589-2999 obtained in 2008 and
2009. The observations indicate that the system is an active Algol binary.
Based on the new data, the mean brightness of the system is decreasing through
the years 2007-2009. The light curves obtained in 2008-2009 are modelled using
the Wilson-Devinney code. We also discussed the light and colour variations of
the system at different orbital phases. Evidence suggests that these brightness
and colour variations are due to the rotation of unevenly distributed starspots
on two components of the system.
