The galaxy presents a disturbed morphology, appearing to be in the late stages of a merger event. The primary body exhibits a somewhat elongated, cigar-like shape. One side has a bluish hue, possibly indicating ongoing star formation in that region. The opposite end shows a yellowish coloration, potentially signifying an older stellar population. The overall structure is irregular and lacks a well-defined disk or spiral arm structure, consistent with post-merger galaxies. A tidal tail or bridge-like feature appears to connect the two previously distinct galaxies, indicating a strong gravitational interaction. This feature seems to be more prominent on one end of the galaxy. There are some indications of dust absorption that may be obscuring some features of the galaxy. Overall, the object shows signs of a recent and significant interaction with another galaxy.
