  In this paper, we have conducted an investigation focused on a segment of the
$Spitzer$ mid-infrared bubble N59, specifically referred to as R1 within our
study. Situated in the inner Galactic plane, this region stands out for its
hosting of five 6.7 GHz methanol masers, as well as numerous compact H II
regions, massive clumps, filaments, and prominent bright rims. As 6.7 GHz
masers are closely linked to the initial phases of high-mass star formation,
exploring regions that exhibit a high abundance of these maser detections
provides an opportunity to investigate relatively young massive star-forming
sites. To characterize the R1 region comprehensively, we utilize
multi-wavelength (archival) data from optical to radio wavelengths, together
with $^{13}$CO and C$^{18}$O data. Utilizing the $Gaia$ DR3 data, we estimate
the distance towards the bubble to be $4.66 \pm 0.70$ kpc. By combining
near-infrared (NIR) and mid-infrared (MIR) data, we identify 12 Class I and 8
Class II sources within R1. Furthermore, spectral energy distribution (SED)
analysis of selected sources reveals the presence of four embedded high-mass
sources with masses ranging from 8.70-14.20 M$_\odot$. We also identified
several O and B-type stars from radio continuum analysis. Our molecular study
uncovers two distinct molecular clouds in the region, which, although spatially
close, occupy different regions in velocity space. We also find indications of
a potential hub-filament system fostering star formation within the confines of
R1. Finally, we propose that the feedback from the H II regions has led to the
formation of prominent Bright Rimmed Clouds (BRC) within our region of
interest.
