We report the discovery of a close-in () warm Neptune with clear transit timing variations (TTVs) orbiting the nearby () active M4 star, TOI-2015. We characterize the planet’s properties using TESS photometry, precise near-infrared radial velocities (RV) with the Habitable-zone Planet Finder (HP) Spectrograph, ground-based photometry, and high-contrast imaging. A joint photometry and RV fit yields a radius , mass , and density for TOI-2015b, suggesting a likely volatile-rich planet. The young, active host star has a rotation period of and associated rotation-based age estimate of . Though no other transiting planets are seen in the TESS data, the system shows clear TTVs of super period and amplitude . After considering multiple likely period ratio models, we show an outer planet candidate near a 2:1 resonance can explain the observed TTVs while offering a dynamically stable solution. However, other possible two-planet solutions – including 3:2 and 4:3 resonance – cannot be conclusively excluded without further observations. Assuming a 2:1 resonance in the joint TTV-RV modeling suggests a mass of for TOI-2015b and for the outer candidate. Additional transit and RV observations will be beneficial to explicitly identify the resonance and further characterize the properties of the system.

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