This galaxy appears to be a spiral galaxy with a prominent disk structure. The spiral arms are well-defined and exhibit a loose winding pattern. The galaxy is observed face-on, revealing a detailed view of the spiral structure. The central bulge is of moderate size. There is a hint of a bar-like structure running through the bulge. The distribution of light suggests a fairly active star formation rate, particularly in the spiral arms. The galaxy does appear to be undergoing some interaction or disturbance, perhaps even a minor merger event, which is causing the galaxy to not appear as clear as others.