The galaxy presents a morphology indicative of an ongoing or recent merger event. Multiple distinct nuclei are observed within a common, diffuse halo. These nuclei exhibit a range of apparent colors, with some appearing more yellow-white and others skewed towards redder hues. The overall form of the galaxy lacks a clear spiral or elliptical structure; rather, it appears as a disturbed, irregular shape. The light distribution across the galaxy is uneven, with brighter concentrations around the nuclei and a fainter, less structured emission extending outwards. The color gradients suggest variations in stellar populations or dust content across the merging system. Tidal features, while not prominent, may be subtly present in the extended, fainter regions of the galaxy. The system is unresolved into distinct stellar populations in this image, suggesting a significant distance or high redshift. Overall, the galaxy appears to be a dynamically active system, likely undergoing significant star formation triggered by the merger event, with potentially moderate rates of star formation based on the colors.
