The galaxy presents as a disk galaxy, observed nearly edge-on. The central bulge appears somewhat prominent and has a yellowish hue, suggesting an older stellar population. The disk itself is relatively thin and exhibits a mottled texture, potentially indicating areas of star formation. The disk is distinctly asymmetrical, with one side appearing brighter and more extended than the other. This asymmetry could be due to tidal interactions with another galaxy, an internal disturbance, or an uneven distribution of interstellar material. There is evidence of possible distortion or warping in the outer regions of the disk. Patches of redder light can be seen dispersed throughout the disk indicating regions of dust or star formation, most apparent on the side of the galaxy which has less density. There are faint irregularities in the disk structure that potentially indicate minor disturbances or interactions occurring.
