The galaxy presents as a flattened, disk-like structure, observed at an oblique angle, suggesting it may be a spiral galaxy. The overall color is a gradient, transitioning from a bluer hue at one end to a redder tone at the opposite extremity. This variation in color could indicate differing stellar populations and star formation activity across the galaxy. A distinct, reddish region is observed offset from the main galactic body. This could be an area of intense star formation, an interacting dwarf galaxy, or a background object aligned along the line of sight. There appears to be a relatively smooth, featureless structure within the disk, with hints of spiral arm structure. No significant signs of major disturbance or ongoing merger events are apparent in the primary structure of the galaxy.
