The galaxy presents a spiral morphology, exhibiting a discernible disk structure. The spiral arms appear somewhat flocculent, with a predominantly two-armed structure. The winding of the spiral arms is relatively loose.

The central bulge is moderately prominent, exhibiting a yellowish hue suggesting an older stellar population. Some bluer regions are observable within the spiral arms, indicating areas of ongoing star formation. There is no evidence of a strong bar structure, but the presence of a weak bar cannot be ruled out.

The overall color of the galaxy suggests it lies within the "green valley", as it displays characteristics of both a star-forming and a passively evolving system. There is indication of a minor disturbance within the structure of the galaxy, but a significant merger is unlikely.
