The galaxy appears to be undergoing a significant merger event. The primary structure displays a roughly elliptical morphology, although this is likely distorted by the interaction. A secondary, smaller structure is closely associated with the main body, suggestive of a tidal interaction or ongoing collision. The color gradient indicates a mix of stellar populations; the central region exhibits a yellowish hue, possibly indicating older stars or dust obscuration, while the outer regions show hints of bluer colors, which could indicate ongoing star formation. There is a noticeable lack of defined spiral arms, further suggesting a disturbed morphology. The overall appearance is somewhat diffuse, indicating that the stellar distribution is not tightly confined, as is typical of post-merger systems.
