The galaxy presents a disturbed morphology, suggestive of an ongoing or recent merger event. Two distinct luminous regions are apparent. One region exhibits a bluer hue, indicative of active star formation and a younger stellar population. The other luminous region displays a yellowish-white color, potentially indicative of an older stellar population. A significant portion of the overall light appears concentrated towards the two luminous regions, with faint tidal features or disrupted arms visible in the periphery. The overall shape appears irregular, lacking a clear spiral or elliptical structure.
