This galaxy exhibits a spiral structure, characterized by prominent, well-defined spiral arms that extend outwards from the central region. These arms appear somewhat flocculent. The arms display a mottled appearance, suggesting regions of active star formation interspersed with areas of dust and gas. 

A bar-like structure appears to traverse the galaxy's core region, bisecting the central bulge. The bulge appears relatively modest in size. The disk of the galaxy is oriented at an angle, providing a view that is neither face-on nor edge-on.

There appear to be some disturbances in the symmetry and morphology of the galaxy. This may be indicative of possible interactions with smaller neighboring galaxies. It exhibits signs of an ongoing or recent merger event. The overall color of the galaxy suggests a mix of stellar populations, with both older, redder stars and younger, bluer stars present.
