The galaxy exhibits a prominent disk structure, viewed at a slight angle. The disk shows evidence of spiral arm morphology, loosely wound and somewhat flocculent. These spiral arms appear traced by regions of active star formation, indicated by their bluer color. The central bulge is moderately sized and shows a yellowish-orange hue, suggesting an older stellar population. There is no strong evidence of a bar structure bisecting the galaxy. The overall color profile suggests ongoing star formation within the disk, while the bulge appears more quiescent. There is no strong visual indication of major disturbances or tidal features that would immediately suggest a recent merger event. The galaxy has a smooth, albeit not perfectly symmetrical, appearance, with minor irregularities that could be interpreted as areas of enhanced star formation or dust obscuration.
