The galaxy presents as a late-type spiral, viewed nearly edge-on. A prominent dust lane bisects the galactic disk, obscuring the central bulge. The bulge exhibits a boxy morphology and appears spheroidal, with moderate concentration. The disk shows distinct blue regions, possibly indicative of on-going star formation. There is little evidence of major tidal disturbances or merging activity. The galaxy is moderately large with an estimated stellar mass of approximately 10^11 solar masses, with a low overall star formation rate.
