  Light curve modeling for the newly discovered system 1SWASP J092328.76+435044
was carried out by using a new BVR complete light curves. A spotted model was
applied to treat the asymmetry of the light curves. The output model was
obtained by means of Wilson-Devinney code, which reveals that the massive
component is hotter than the less massive one with about \Delta T ~ 400K. A
total of 8 new times of minima were estimated. The evolutionary state of the
system components was investigated based on the estimated physical parameters.
