The galaxy presents as a spiral type, characterized by distinct, albeit somewhat ill-defined, spiral arms. A central bulge is present, appearing moderately prominent within the galaxy's overall structure. The arms exhibit a bluer hue, suggestive of ongoing star formation. Dust lanes are present, though not sharply defined, contributing to the observed morphology. There is no strong indication of a prominent bar structure. The overall appearance of the galaxy suggests it is relatively undisturbed.
