We present results from multiwavelength observations of the BL Lacertae object 1ES 1741+196, including results in the very-high-energy $gamma$-ray regime using the Very Energetic Radiation Imaging Telescope Array System (VERITAS). The VERITAS time-averaged spectrum, measured above 180 GeV, is well-modelled by a power law with a spectral index of $2.7pm0.7_{mathrm{stat}}pm0.2_{mathrm{syst}}$. The integral flux above 180 GeV is $(3.9pm0.8_{mathrm{stat}}pm1.0_{mathrm{syst}})times 10^{-8}$ m$^{-2}$ s$^{-1}$, corresponding to 1.6% of the Crab Nebula flux on average. The multiwavelength spectral energy distribution of the source suggests that 1ES 1741+196 is an extreme-high-frequency-peaked BL Lacertae object. The observations analysed in this paper extend over a period of six years, during which time no strong flares were observed in any band. This analysis is therefore one of the few characterizations of a blazar in a non-flaring state.
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