The galaxy presents as a complex system, potentially undergoing interaction or possessing an unusual morphology. The core region exhibits a bright, yellowish hue, suggesting an older stellar population. Emanating from this central region is an extended feature, appearing to be composed of greenish and reddish tints. The greenish components might indicate regions of active star formation, while the reddish component may indicate a substantial amount of dust and gas in the galaxy. A notable disturbance seems to be present in the main structure of the galaxy, suggesting an on-going merger or significant gravitational interactions. The overall shape appears asymmetrical, with the aforementioned extension departing significantly from a smooth elliptical profile. This system does not clearly exhibit a classical spiral or elliptical morphology.
