We introduce a method for imaging the earthquake source dynamics from the inversion of ground motion records based on a parallel genetic algorithm. The source model follows an elliptical patch approach and uses the staggered-grid split-node method to simulate the earthquake dynamics. A statistical analysis is used to estimate errors in both inverted and derived source parameters. Synthetic inversion tests reveal that the average rupture speed (V r ), the rupture area, and the stress drop (Δτ) may be determined with formal errors of~30%,~12%, and~10%, respectively. In contrast, derived parameters such as the radiated energy (E r ), the radiation efficiency (η r ), and the fracture energy (G) have larger errors, around~70%, 40%, and~25%, respectively. We applied the method to the M w 6.5 intermediate-depth (62 km) normal-faulting earthquake of 11 December 2011 in Guerrero, Mexico. Inferred values of Δτ = 29.2 ± 6.2 MPa and η r = 0.26 ± 0.1 are significantly higher and lower, respectively, than those of typical subduction thrust events. Fracture energy is large so that more than 73% of the available potential energy for the dynamic process of faulting was deposited in the focal region (i.e., G = (14.4 ± 3.5) × 10 14 J), producing a slow rupture process (V r /V S = 0.47 ± 0.09) despite the relatively high energy radiation (E r = (0.54 ± 0.31) × 10 15 J) and energy-moment ratio (E r /M 0 = 5.7 × 10). It is interesting to point out that such a slow and inefficient rupture along with the large stress drop in a small focal region are features also observed in both the 1994 deep Bolivian earthquake and the seismicity of the intermediate-depth Bucaramanga nest.