This galaxy appears to be a relatively small, disk-shaped system, observed nearly edge-on. The central bulge is not very prominent and the galaxy appears somewhat flat. The color gradient across the galaxy suggests some degree of ongoing star formation, with bluer colors more prevalent throughout the galaxy. The overall smoothness of the light distribution indicates a lack of strong spiral arm structure or significant dust lanes. There might be some minor tidal disturbances or interactions with other objects, though they are not pronounced. The galaxy does not appear to be undergoing a major merger, though some minor disturbances may be present. It also has some light with a red hue around it.
