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

Light Curve Modelling and Evolutionary Status of the Short Period Binary 1SWASP J092328.76+435044