This galaxy exhibits a clear disk morphology, viewed nearly edge-on. The central bulge is prominent and appears relatively smooth. Some evidence of internal structure within the disk is present, although details are limited by the image resolution. The galaxy demonstrates detectable star formation, indicated by the presence of some slightly bluer regions, suggesting recent or ongoing stellar genesis, and also redder areas indicating regions of hydrogen-alpha emission. However, it is not undergoing vigorous starburst activity. The overall structure does not appear significantly disturbed, showing no signs of a recent major merger. There is a slight asymmetry in the intensity along the galactic plane and disk. This could mean it has had a minor disturbance, but is overall undisturbed.
