The galaxy presents as a spiral type, observed at an angle somewhat close to edge-on, though the spiral arms are still visible. The central bulge is moderately sized and possesses a yellowish hue, suggesting an older stellar population. The spiral arms appear tightly wound and are predominantly blue, indicative of ongoing star formation. The arms appear somewhat disturbed, and there is no strong central bar visible. The color suggests an intermediate stage of star formation. No significant signs of mergers or tidal disturbances are immediately apparent.
