  In previous works, we have investigated the star-forming region G29.96$-$0.02
where the massive young stellar object (MYSO) G29.862$-$0.0044 (hereafter G29)
is embedded in a hot molecular core. In one of them, of multiwavelength nature,
using data from the Atacama Submillimeter Telescope Experiment (ASTE), data
from the Atacama Large Millimeter Array (ALMA), and photometric data from
NIRI-Gemini, G29 was investigated at different spatial scales. However, the
intriguing morphology of G29 in the near-infrared, together with the
distribution of the associated molecular gas, reveals that the star-formation
scenario is far from being understood. This work incorporates the analysis of
the emission of several molecular lines acquired with ALMA that were not
previously examined (eg.,~CH$_{3}$OH, HC$_{3}$N, H$_{ 2}$CO, C$^{34}$S,
H$_{2}$CS) as well as a new determination of the temperature of the region.
Additionally, we present the progress of results obtained through new
observations in the near-infrared, in this case spectroscopic, using
NIFS-Gemini, and in radio continnum obtained with the Karl G. Jansky Very Large
Array (JVLA). This research allows us to carry out a detailed chemical study of
the region, which will contribute to the understanding of the physical
processes involved in the high-mass star formation.
