The galaxy presents as a spiral galaxy, viewed at a slight angle, but approaching face-on. The spiral arms are well-defined, emanating from a central bulge, and show evidence of active star formation, indicated by the clumpy, blueish regions within the arms. The arms appear somewhat tightly wound near the center and loosen further out. The central bulge is a moderate size, and appears to be relatively smooth. The overall color of the galaxy suggests a mix of older stellar populations in the bulge, and younger, hotter stars concentrated in the arms. No obvious bar structure is visible. There is no clear evidence of any major merger events or significant disturbances in its morphology.