Comparison of the host galaxy properties of GRB 140506A (large red dot) to 20 other GRB host galaxies at z< 1 (small blue dots) with metallicity measurements from Krühler et al. (2015). From left to right the metallicity of each individual host galaxy is shown as a function of: A_V, SFR and σ, measured from emission line diagnostics. The dotted, horizontal line denotes the solar metallicity abundunce (Asplund et al. 2009). The physical properties of the host galaxy of GRB 140506A is inconspicuous, compared to the other GRB host galaxies at z< 1.