The galaxy presents a morphology suggestive of an ongoing or recent merger. The primary body of the galaxy appears distorted, exhibiting an elongated shape with a possible dual core or nucleus. The colour gradient indicates the presence of both older stellar populations, evident in the redder hues, and regions of active star formation, as suggested by the bluer tones and luminosity. There are no clear spiral arm structures or a defined disk, further supporting the hypothesis of a disturbed or transitional morphological state potentially induced by the merger event. The overall visual impression indicates a galaxy of significant mass and luminosity undergoing a dynamic evolutionary process.
