Lomb-Scargle periodogram of the out-of-eclipse TESS light curve. We measure the rotational modulation in the TESS light curve and obtain a periodicity of 2.013 ± 0.076 d, which is consistent with synchronous rotation. The most significant period is marked in both the plot and the inset with the vertical red lines. The inset shows the structure around the most significant peak, with its width determining the uncertainty in the rotation period.