  Triple AGN systems are expected to be the result of the hierarchical model of
galaxy formation. Since there are very few of them confirmed as such, we
present the results of a new study of the triple-AGN candidate SDSS
J102700.40+174900.8 (center nucleus) through observations with
$\it{GTC}$-$\it{MEGARA}$ Integral Field Unit. 1D and 2D analysis of the line
ratios of the three nuclei allow us to locate them in the EW(H$\alpha$) vs.
[Nii] /H$\alpha$ diagram. The central nucleus is found to be a retired galaxy
(or fake AGN). The neighbors are found to be a strong AGN (southeastern
nucleus, J102700.55+174900.2) compatible with a Sy2 galaxy, and a weak AGN
(northern nucleus, J102700.38+174902.6) compatible with a LINER2. We find
evidence that the neighbors constitute a dual AGN system (Sy2-LINER2) with a
projected separation of 3.98 kpc in the optical bands. The H$\alpha$ velocity
map shows that the northern nucleus has an H$\alpha$ emission with a velocity
offset of $\sim$-500 km s$^{-1}$, whereas the southeastern nucleus has a
rotating disk and H$\alpha$ extended emission at kpc scales. Chandra archival
data confirm that the neighbors have X-ray (0.5-2) keV and (2-7) keV emission,
whereas the center nucleus shows no X-ray emission. A collisional ring with
knots is observed in the HST images of the southeastern nucleus. These knots
coincide with star formation regions that along with the ring are predicted in
a head-on collision. In this case, the morphology changes are probably due to a
minor merger that was produced by the passing of the northern through the
southeastern nucleus.
