The eclipsing binary XZ Andromedae has been the subject of many observing campaigns, due to variability of its orbital period and the interesting mechanisms causing the change. We therefore observed this star during the period October-November 2021. We determined the current orbital period (P = 1.357308 (18) d), and using transformed standard BVI magnitudes, constructed a model of the eclipsing binary using the PHOEBE (Physics of Eclipsing Binaries) and Binary Maker 3 software packages to compare with results from previous studies. The model that best fit the data suggests that XZ And is a semidetached system with the secondary filling the Roche Lobe. The parameters fit of the primary (T_1 = 9393 K, mass M_1 = 2.1 solar masses, and radius R_1 = 2.2 solar radii) are indicative of a A1V main sequence star, while the secondary's parameters (T_2 = 5334, M_2 = 1.02, and R_2 = 2.40) point to a star in a more advanced evolutionary status.
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