The galaxy exhibits a disturbed morphology suggestive of an ongoing or recent merger event. The central region is dominated by a relatively bright, amorphous structure, possibly representing the combined nuclei of the progenitor galaxies. There is evidence of tidal features such as faint streams or tails extending from the main body, indicating gravitational interaction. The color is predominantly blue, indicative of recent star formation. There are no clear spiral arms or a well-defined disk. A small, green area on the left edge appears as a possible star forming region. There is a possibility of a major disruption or merger being present.
