Transverse stability governs the safety and operability of ships, and roll—the rotation about the longitudinal axis—produces the largest lateral oscillations, affecting crew comfort, cargo safety and structural loads. Reduced-scale nautical models offer a low-cost route to study this behavior, yet quantitative roll models and simple, space-constrained stabilization solutions for competition models remain scarce. This work models the free roll of the Jaraqui nautical model as a linear second-order (mass–spring–damper) system, valid for small heel angles (sin φ ≈ φ). The equation of motion was cast in state-space form and integrated in MATLAB with the ode45 (Runge–Kutta 4/5) solver. A parametric study varied the damping ratio ζ from 0.02 to 0.50 at a natural frequency ωn = 1 rad/s and an initial heel of 10°; the damped period, 2% settling time and logarithmic decrement were computed. The simulated response reproduced the expected exponentially decaying oscillation. Increasing ζ from 0.02 to 0.50 shortened the 2% settling time from ≈200 s to 8 s and raised the logarithmic decrement from 0.13 to 3.63, while the damped period grew only 16%. A passive internal-pendulum stabilizer was then sized conceptually: the central hull region near the longitudinal center of gravity was identified as the installation site, with a 90–110 mm arm, a 150–250 g mass and ±20° travel, subject to a tuning condition ωpendulum ≈ ωroll for effective energy transfer. The linear model captures the essential roll physics and provides a design-oriented basis for a low-cost passive stabilizer; experimental identification of the true roll frequency and prototype testing are the next steps.