This galaxy exhibits a prominent, well-defined spiral structure. The arms appear flocculent, with a somewhat patchy distribution of star formation regions. Two distinct arms are readily visible, tightly wound around the galactic center.

A central bulge is apparent, displaying a moderate size and exhibiting a yellowish hue, possibly indicating an older stellar population. There is evidence of a bar structure extending through the central region. The bar seems relatively strong.

Overall, the galaxy shows no immediately obvious signs of a major merger, although minor disturbances may be present in the spiral arm structure. It seems to be relatively undisturbed.
