The galaxy presents as a somewhat elliptical structure, viewed at a relatively high inclination. The core region appears bright and concentrated, suggesting a high stellar density. The color distribution indicates a redder central bulge transitioning to bluer outer regions, potentially indicative of younger stellar populations in the disk. There's a hint of possible dust lanes or patchy extinction bisecting the galaxy, though this could be an artifact. There also may be slight merging disturbances visible in the morphology of the galaxy. Overall, the galaxy exhibits a relatively smooth appearance with a noticeable central bulge and a disk structure, suggesting a spiral galaxy undergoing some sort of interaction.
