We present the complete set of physical and geometrical parameters of the visual close binary system GJ 9830 for the first time by using Al-Wardat ’ s complex method . This method combines magnitude difference from speckle interferometry , synthetic spectral energy distributions of the binary components which are constructed depending on grids of Kurucz blanketed models ( Atlas9 ) , along with the orbital solution by using Tokovinin ’ s dynamical method to estimate the parameters of the individual components . The analysis of the system by using synthetic photometry resulted in the following set of parameters : T _ { eff . } = 6220 \pm 100 K , log~ { } g = 4.30 \pm 0.12 , R = 1.10 \pm 0.08 R _ { \odot } for the primary component and T _ { eff . } = 4870 \pm 100 K , log~ { } g = 4.60 \pm 0.11 , R = 0.709 \pm 0.07 R _ { \odot } for the secondary component . The recently published dynamical parallax from Gaia space mission was used to calculate the total mass of the binary system as 1.75 \pm 0.06 \mathcal { M } _ { \odot } which coincides with those estimated by using Al-Wardat ’ s method as \mathcal { M } ^ { A } = 1.18 \pm 0.10 \mathcal { M } _ { \odot } , \mathcal { M } ^ { B } = 0.75 \pm 0.08 \mathcal { M } _ { \odot } . The analysis of the system reveals that both components belong to main sequence stars with an age around 1.4 \pm 0.50 Gyr . The evolutionary tracks and isochrones of the system ’ s components are discussed , and the fragmentation process is suggested as the most likely process for the formation of the system .