The galaxy presents as an edge-on disk galaxy with a prominent central bulge. The bulge exhibits a somewhat boxy morphology. The disk appears relatively smooth and extended. The galaxy is approximately 4.7 kpc in radius. There's evidence of ongoing star formation, though possibly at a moderate specific star formation rate. The galaxy does not appear to be undergoing any major merging activity, though minor tidal disturbances cannot be completely ruled out. The color gradient suggests a possible dust lane obscuring the central region of the disk.
