The galaxy presents as a system undergoing, or having recently undergone, a significant merger event. There are two distinct, somewhat unresolved luminous cores that display differential color. One core exhibits a bluer spectral signature, indicative of recent or ongoing star formation, whereas the other exhibits a redder hue, potentially arising from an older stellar population or significant dust obscuration. Extensive tidal features and/or a complex interacting morphology appear to exist, with some degree of distortion from a smooth elliptical shape. This galaxy has a moderate spatial extent on the sky.
