This galaxy appears to be undergoing a significant interaction or merger. The primary galaxy body presents a smooth, elliptical morphology with a concentrated central bulge region exhibiting a yellow-orange hue, indicative of an older stellar population. A tidal tail extends outwards, displaying a bluer color. The presence of the tidal tail suggests relatively recent or ongoing star formation. The main body is estimated to be a few kiloparsecs in radius. The lower luminosity region is distinctly bluer, and shows signs of irregular morphology. The system is likely undergoing a major disruption.
