  We have studied the nuclear region of the previously detected dual AGN system
in the galaxy pair IRAS 05589+2828 and 2MASX J06021107+2828382 through new
optical spectroscopy observations, along with radio and X-ray archival data.
Our multiwavelength data strongly suggest that the Sy1 \iras\,
(z=0.0330$\pm$0.0002) conforms to a dual AGN system with the Sy2 \twomas\,
(z=0.0334$\pm$0.0001) with a projected separation obtained from the radio data
of 20.08\arcsec\, ($\sim$13.3\,kpc). Analysis of the optical spectra reveals a
faint narrow extended emission from H$\alpha$ and [OIII] amidst the two AGN,
supporting evidence for an ongoing merger. \iras\, is a double component narrow
emission line AGN, with complex broad Balmer emission line profiles that
clearly show a strong red-peaklet with a velocity shift of
$\sim$3500\,km\,s$^{-1}$. The black hole mass estimates of \iras\, and
\twomas\, are log\,M$\rm_{BH}$\,=\,8.59\,$\pm$\,0.14 (M$_\odot$) and
log\,M$\rm_{BH}$\,=\,8.21$\pm$0.2 (M$_\odot$), respectively. In the X-ray
bands, \iras\, is compatible with a Type 1 object, showing both spectral and
flux variability. \chandra\, data of 2MASX\,J06021107+2828382 allowed us to
measure a high hardness ratio in this source, providing evidence for a Type 2
AGN. The 22 GHz image obtained with the {\it Karl G. Jansky Very Large Array}
has revealed that both AGN are compact radio objects with spectral indices
-0.26$\pm$0.03 and -0.70$\pm$0.11, confirming for the first time its dual AGN
nature in the radio bands.
