The galaxy presents a somewhat amorphous, though largely centralized structure, with an apparent disk-like feature embedded within it. It exhibits a moderate degree of overall smoothness, with some regions appearing more diffuse than others. The core region appears slightly brighter with a distinct cyan hue. Surrounding the brighter core are areas of faint red emission as well as hints of spiral structure. The galaxy does not appear perfectly rounded; it exhibits a slight deviation from a circular shape. It exhibits signs of potential interaction with another galaxy based on the disturbances visible within its structure. There are also some signs that the merging event may have a larger effect than minor disturbances.
