This galaxy appears to be undergoing a significant interaction or merger. There are two distinct, bright cores visible, suggesting either two galaxies in the process of merging or a single galaxy with a highly disturbed nucleus. The overall shape is irregular and elongated, with some indications of tidal features extending outwards, particularly to the upper right. The light profile suggests a relatively smooth stellar distribution within each core region. There are subtle color gradients with some areas appearing yellower or redder than others. This color variation may suggest differences in stellar populations and dust content within the galaxy. The galaxy does not present a clear spiral or elliptical morphology, indicating a dynamically disturbed system.
