The galaxy presents as a somewhat elongated, disk-like structure viewed at a high inclination. It exhibits a diffuse central bulge which gradually fades into the disk. There is evidence of spiral arm structure, although it is not sharply defined. Patches of bluer light, indicative of recent star formation, are visible interspersed with regions of older, redder stellar populations. The overall color suggests a relatively quiescent galaxy with a low rate of star formation. There is no obvious sign of any major disturbance or ongoing merger event. Some minor asymmetry may be present. The galaxy appears relatively smooth.
