The galaxy presents as a somewhat irregular structure with a reddish-yellow hue, suggestive of an older stellar population and potentially significant dust obscuration. There appears to be a bright central region. The galaxy displays a significant degree of disturbance in its morphology, hinting at a possible ongoing or recent merger event. The overall shape is elongated, with less defined spiral arms. It exhibits a significant amount of blue light, and the color suggests it's undergoing active star formation. Luminous regions are present throughout.