  IGR J09026-4812 was discovered by INTEGRAL in 2006 as a new hard X-ray
source. Thereafter, an observation with Chandra pinpointed a single X-ray
source within the ISGRI error circle, showing a hard spectrum, and improving
its high-energy localisation to a subarcsecond accuracy. Thus, the X-ray source
was associated to the infrared counterpart 2MASS J09023731-4813339 whose JHKs
photometry indicated a highly reddened source. The high-energy properties and
the counterpart photometry suggested a high-mass X-ray binary with a main
sequence companion star located 6.3-8.1 kpc away and with a 0.3-10 keV
luminosity of 8e34 erg/s. New optical and infrared observations were needed to
confirm the counterpart and to reveal the nature of IGR J09026-4812. We
performed optical and near infrared observations on the counterpart 2MASS
J09023731-4813339 with the ESO/NTT telescope on March 2007. We achieved
photometry and spectroscopy in near infrared wavelengths and photometry in
optical wavelengths. The accurate astrometry at both optical and near infrared
wavelengths confirmed 2MASS J09023731-4813339 to be the counterpart of IGR
J09026-4812. However, the near infrared images show that the source is
extended, thus excluding any Galactic compact source possibility. The source
spectrum shows three main emission lines identified as the HeI lambda 1.0830
micron line, and the HI Pa_beta and Pa_alpha lines, typical in galaxies with an
active galactic nucleus. The broadness of these lines reached values as large
as 4000 km/s pointing towards a type 1 Seyfert galaxy. The redshift of the
source is z=0.0391(4). Thus, the near infrared photometry and spectroscopy
allowed us to classify IGR J09026-4812 as a Seyfert galaxy of type 1.
