This galaxy exhibits a complex morphology, appearing to be in a state of interaction or merger. The primary body of the galaxy shows a somewhat disrupted structure, with an overall elongated shape. The central region is relatively bright and concentrated. There is evidence of tidal features extending from the main body, possibly indicative of gravitational interactions with another galaxy. The galaxy exhibits a bluer hue in some regions, potentially suggesting ongoing star formation. A secondary, smaller object is nearby, which may be a dwarf galaxy or another component involved in the interaction. Some regions display reddish tones, which may be older stellar populations or dust obscuration.
