The galaxy presents as a spiral type, observed at an oblique angle but not fully edge-on. There is a defined central bulge region that is more luminous than the rest of the galaxy. The bulge appears yellowish-white. Spiral arms are visible, though not sharply defined. The arms have a fragmented appearance, displaying a mottled structure with a bluish-white hue, which could indicate regions of active star formation. There are approximately three spiral arms that can be easily discerned. The winding of the arms appears to be relatively tight. A faint bar structure may be present across the central region. There is no clear indication of a major merger event, though a minor disturbance cannot be ruled out based on the morphology.
