  We present an orbital solution study for the newly discovered system 1SWASP
J080150.03+471433.8 by means of new CCD observations in VRI bands. Our
observations were carried out on 25 Feb. 2013 using the Kottamia optical
telescope at NRIAG, Egypt. 12 new times of minima were estimated and the
observed light curves were analysed using the Wilson-Devinney code. The
accepted orbital solution reveals that the primary component of is more massive
and hotter than the secondary one by about 280K. The system is an over-contact
one with fillout ratio ~ 29% and is located at a distance of 195 Pc. The
evolutionary status of the system is investigated by means of stellar models
and empirical data.
