The galaxy presents a spiral morphology. It is observed at a low inclination, offering a near face-on view. The spiral arms are well-defined, exhibiting a grand design structure. These arms appear somewhat flocculent, with varying degrees of brightness along their lengths. The central bulge is moderately sized and exhibits a yellowish color, potentially indicative of an older stellar population. A bar structure appears prominent across the central region of the galaxy. Dust lanes are faintly visible within the spiral arms. The overall color profile suggests ongoing star formation, particularly in the arms. There is no obvious evidence of a major ongoing merger, although some minor disturbances within the disk cannot be ruled out.
