The galaxy appears to be in the late stages of a major merger. The central region exhibits a complex structure, possibly with multiple nuclei. The morphology is highly disturbed, indicating strong tidal interactions. There's evidence of significant disruption to the galaxy's original form, with no clear spiral arms or defined disk. The overall color is yellowish-red, suggesting an older stellar population with ongoing or recent star formation. The relatively high luminosity of the galaxy may be due to increased activity from the merger. A faint halo of diffuse light surrounds the main body, potentially composed of stripped stars and gas.
