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The distance to the source was determined from its annual parallax which was measured to be 3.06$\\pm$0.04 mas, corresponding to a distance of 327$\\pm$4\\,pc. Our observations revealed the distribution and internal kinematics of H$_2$O masers in T~Lep, and we derived a source systemic motions of 14.60$\\pm$0.50 mas yr$^{-1}$ and $-$35.43$\\pm$0.79 mas yr$^{-1}$ in right ascension and declination, respectively. 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