This galaxy presents as a flattened, disk-like structure observed nearly edge-on. The central region appears brighter and more concentrated, possibly indicating a bulge. A dust lane bisects the galaxy, obscuring the central regions and contributing to a mottled appearance. There are no clear spiral arm structures visible. The outer regions of the disk appear fainter and more diffuse. There is a second, smaller galaxy in close proximity. Based on the disturbances, the galaxy could be undergoing a minor merger event.
