The galaxy appears to be undergoing a significant interaction or merger. Its overall morphology is disturbed, exhibiting an irregular shape rather than a well-defined spiral or elliptical structure. There are hints of tidal features, perhaps faint tails or bridges of stars and gas extending from the main body, though these are not sharply defined.

Color variations are present throughout the system, with some regions displaying a reddish hue, potentially indicating older stellar populations or dust obscuration, while other areas show bluer tints, suggestive of ongoing star formation. The light is generally concentrated towards the center, but there are multiple condensations or nuclei visible, supporting the merger hypothesis. The central region itself shows multiple lobes of light, instead of a single central point.

The overall smoothness of the galaxy is compromised by the disturbed structure, though it does have an overall degree of symmetry, which hints at the intermediate stages of a merger in process.
