The galaxy presents as a disk galaxy, viewed nearly edge-on from our perspective. It exhibits a prominent central bulge region which appears yellowish in color. The disk itself demonstrates a mottled texture, with subtle color variations suggesting regions of differing stellar populations or dust obscuration. The outer edges of the disk appear somewhat diffuse, fading into the background sky. There is evidence of some degree of disturbance or ongoing interaction, manifested as a slight asymmetry in the disk and possibly subtle tidal features extending away from the main body of the galaxy. The absence of strong spiral arm structures suggests a relatively smooth stellar distribution within the disk.
