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Photometric data were used to perform the first light curve analysis of theV0610 Vir binary system. We extracted the minima from our observations andcompiled the literature, which was few in number. Therefore, we performedcomputations using the reference ephemeris and presented a new ephemeris andO-C diagram with a linear fit. Light curve analysis was performed using thePHOEBE Python code and the Markov chain Monte Carlo (MCMC) approach. Theassumption of a cold spot was required due to the asymmetry in the lightcurve's maxima. The analysis shows that V0610 Vir is a contact binary systemwith a fillout factor of 0.085, a mass ratio of 0.998, and an inclination of70.65deg. The absolute parameters of the system were estimated based on theGaia DR3 parallax method. The results show that the system is a Low-MassContact Binary (LMCB) with a total mass lower than 0.8(M_Sun). The location ofthe stars was shown in the M-L and M-R diagrams.

First Light Curve Study of the Low Mass Contact Binary V0610 Vir