The galaxy presents a disturbed morphology, likely a result of an ongoing or recent interaction. There is an elongation to the overall shape. The core region exhibits a bright and concentrated central component. A secondary, less luminous condensation is observed to the right of the core, potentially a satellite galaxy or a region of enhanced star formation triggered by the interaction. There is a slight indication of faint spiral arm structure emanating from the central core, though it is heavily disrupted. Overall, the galaxy exhibits a yellowish-red color, indicative of an older stellar population with a lower rate of active star formation.
