The galaxy presents as an intermediate spiral galaxy. The overall color profile suggests a population of relatively mature stars. It exhibits a moderate central bulge with a prominent disk. Faint spiral arm structures can be discerned, though they appear somewhat tightly wound and not very well defined. There appears to be little evidence of active star formation. No strong bar structure is visible. The disk is oriented nearly face-on, allowing for a good view of the spiral structure. There is a possibility of a minor interaction or disturbance within the galaxy, though it appears mostly undisturbed. 
