The galaxy appears to be undergoing a significant merger or interaction with another galaxy. There are two distinct, bright cores visible, suggestive of the nuclei of two interacting galaxies. One nucleus appears more yellow, while the other is more white, suggesting differing stellar populations or dust content. The overall shape is highly irregular, lacking any clear spiral or elliptical structure, consistent with ongoing gravitational disruption. Faint tidal features or extended stellar halos might be present, but are difficult to distinguish from the background noise at this resolution. There is evidence of ongoing or recent star formation within the system, possibly enhanced by the merger event.
