It is an early type star of the carbon sequence (WCE) classified as WC5.
No x-rays have been detected from WR 114, which would be expected by a close hot companion.
The properties of a Wolf Rayet star are typically reported at an "inner boundary" of the wind, arbitrarily set at an optical depth of 20.
[3][7] The stellar wind from WR 114 is powered by the high temperature and luminosity to a speed of 2,000 km/s.
WR 114 is listed in the Catalogue of galactic Wolf Rayet stars at around 6,500 light years, but more recent modelling estimates it to be brighter and hence probably more distant.