The galaxy presents as a face-on or nearly face-on spiral, exhibiting a flocculent spiral structure with poorly defined arm segments. These fragmented arms are bluer in color, suggesting regions of active star formation. There is evidence of a weak central bar structure. The bulge is relatively small or non-existent with a dim center. The overall morphology indicates an unorganized appearance and could be undergoing or have undergone a merger event, indicated by irregular features and a non-smooth disk. There are some features that indicate minor disturbances or gravitational interactions within the galaxy.
