A possible binary AGN in Mrk\,622?
  Mrk\,622 is a Compton Thick AGN and a double-peaked narrow emission line
galaxy, thus a dual AGN candidate. In this work, new optical long-slit
spectroscopic observations clearly show that this object is rather a triple
peaked narrow emission line galaxy, with both blue and red shifted narrow
emission lines, as well as a much narrower emission line centred at the host
galaxy systemic velocity. The average velocity offset between the blue and red
shifted components is $\sim$500 km\,s$^{-1}$, which is producing the apparent
double-peaked emission lines. These two components are in the loci of AGN in
the Baldwin, Phillips \& Terlevich (BPT) diagrams and are found to be spatially
separated by $\sim$76 pc. Analysis of the optical spatially resolved
spectroscopic observations presented in this work favours that Mrk\,622 is a
system consisting of a Composite AGN amidst a binary AGN candidate, likely the
result of a recent merger. This notwithstanding, outflows from a starburst, or
single AGN could also explain the triple nature of the emission lines.
