This galaxy exhibits a distinct, elongated morphology. It appears to be a disk galaxy viewed edge-on. The central bulge is not particularly prominent, but there's a subtle brightening along the major axis indicating the presence of older stars. The disk shows hints of dust lanes, contributing to the galaxy's reddish color. The disk also has a smooth appearance. The is no current evidence of any major mergers. The estimated stellar mass suggests the galaxy is of intermediate size. Based on its star formation properties, it is currently forming stars. The specific star formation rate suggest star formation is relatively low considering its stellar mass.
