The galaxy presents as a spiral galaxy with a notable disk. The disk component dominates the overall structure, appearing significantly larger than the bulge. A moderately sized bulge is observed with a yellow-white color, indicating an older stellar population. The spiral arms appear to be tightly wound around the galactic center. The disk exhibits a bluish hue, which is indicative of ongoing star formation. The galaxy does not display signs of any major disturbances, or a recent major merger event. There is some minor irregularity visible, indicating some potential minor disturbances.
