The galaxy presents as a spiral structure, with prominent, well-defined arms emanating from a central bulge. The arms exhibit a tightly wound morphology, showing a gradient in color, with bluer regions indicating areas of active star formation. The central bulge appears relatively bright and concentrated. There is evidence for a bar-like structure extending from the central bulge. No major disturbances or signs of ongoing merging events are readily apparent, although some subtle irregularities within the arms may suggest minor interactions. The disk is oriented at an angle.
