The galaxy presents as a relatively smooth, centrally concentrated object. It has a disk like shape with a major axis that is approximately four times longer than its minor axis. This indicates that the galaxy is not close to face-on. There is evidence of a central bulge. The galaxy has a blueish tint. There appear to be some minor disturbances or interactions occurring within the galaxy's structure, slightly disrupting its smooth appearance. No obvious signs of spiral arm structures are observed. Overall, the galaxy does not appear to be undergoing a major merger or significant disruption.
