This galaxy exhibits a clear disk-like structure viewed edge-on. A prominent central bulge dominates its luminosity profile. The bulge appears to be generally rounded, with a concentration of older stellar populations as indicated by the redder color. The disk component is thinner than the bulge, and shows hints of dust lanes obscuring some of the light. The overall color suggests that star formation is not widespread but potentially concentrated in localized regions within the disk. There is no obvious evidence of ongoing mergers or significant tidal disturbances in the immediate vicinity of the galaxy, though minor internal structures are hard to resolve.
