  We study the stellar populations and assembly of the nearby spiral galaxy NGC
2903's bulge, bar, and outer disc using the VIRUS-P Exploration of Nearby
Galaxies IFS survey. We observe NGC 2903 with a spatial resolution of 185 pc
using the Mitchell Spectrograph's 4.25 arcsec fibres at the 2.7 Harlan J. Smith
telescope. Bulge-bar-disc decomposition on the 2MASS Ks-band image of NGC 2903
shows that it has ~6%, 6%, and 88%, of its stellar mass in the bulge, bar, and
outer disc, respectively, and its bulge has a low Sersic index of ~0.27,
suggestive of a disky bulge. We perform stellar population synthesis and find
that the outer disc has 46% of its mass in stars >5 Gyr, 48% in stars between 1
and 5 Gyr, and <10% in younger stars. Its stellar bar has 65% of its mass in
ages 1-5 Gyr and has metallicities similar to the outer disc, suggestive of the
evolutionary picture where the bar forms from disc material. Its bulge is
mainly composed of old high-metallicity stars though it also has a small
fraction of young stars. We find enhanced metallicity in the spiral arms and
central region, tracing areas of high star formation as seen in the Halpha map.
These results are consistent with the idea that galaxies of low bulge-to-total
mass ratio and low bulge Sersic index like NGC 2903 has not had a recent major
merger event, but has instead grown mostly through minor mergers and secular
processes.
