The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction or merger. The central region appears elongated and distorted, with an irregular distribution of light. The galaxy appears to be composed of multiple components, possibly remnants of the merging galaxies, with varying degrees of color and intensity. The luminosity suggests a galaxy of considerable size and mass. There is evidence of regions with enhanced star formation, particularly toward one end, indicated by a redder hue, contrasting with bluer areas. The overall appearance points towards a complex system undergoing significant evolutionary changes.
