The galaxy presents as a spiral galaxy with tightly wound arms. It appears to have a moderate-sized bulge. The galaxy exhibits a central concentration of light, possibly indicative of an older stellar population in the bulge. The spiral arms appear to have hints of active star formation. The overall color suggests a relatively mature galaxy, though hints of blue indicate ongoing, but not intense, star formation. The galaxy does not show evidence of a strong bar structure. No major disturbances or signs of merging are apparent in the galaxy's morphology. The dust lanes are hard to make out but it looks like there are some. The disk is not edge-on, it has a more face-on orientation to our view.
