The galaxy appears to be a spiral, viewed at an angle. The overall color of the galaxy is bluish-green, suggesting the presence of recent star formation. There are several bright knots scattered throughout, indicative of HII regions or young star clusters. The central region appears smoother and more diffuse, possibly indicating an older stellar population in the bulge. There is some evidence of dust lanes or dark regions, particularly in the lower regions. The spiral arms are not well-defined, and appear somewhat flocculent, suggesting a disordered or disturbed morphology. There is a slight suggestion of a faint tidal tail or minor disturbance on the left edge, indicating a possible interaction or merger event.
