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A global analysis of the system shows that the host star is an evolved subgiant star with $T_{\\rm eff} = 5370\\pm51$ K, $M_{*} = 1.438_{-0.052}^{+0.061} M_{\\odot}$, $R_{*} = 2.72_{-0.17}^{+0.21} R_{\\odot}$, log $g_*= 3.727_{-0.046}^{+0.040}$, and [Fe/H]$ = 0.180\\pm0.075$. The planet is a low-mass gas giant in a $P = 4.736529\\pm0.00006$ day orbit, with $M_{P} = 0.195\\pm0.018 M_J$, $R_{P}= 1.37_{-0.12}^{+0.15} R_J$, $\\rho_{P} = 0.093_{-0.024}^{+0.028}$ g cm$^{-3}$, surface gravity log ${g","authors_text":"Allyson Bieryla, Andrew W. Howard, Benjamin J. Fulton, B. Scott Gaudi, Christopher Stockdale, Daniel Bayliss, David H. Sliski, David James, David W. Latham, Dimitri Mawet, Eric L. N. Jensen, George Zhou, Howard Isaacson, Howard M. Relles, Ivan Curtis, Jason D. Eastman, Jason T. Wright, John Asher Johnson, John Kielkopf, Jonathan Labadie-Bartz, Joseph E. Rodriguez, Joshua Pepper, Kaloyan Penev, Karen A. Collins, Keivan G. Stassun, Knicole D. Col\\'on, Michael B. 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