The galaxy presents as a likely interacting system, potentially undergoing a major merger. Morphologically, it shows a disturbed structure, with a noticeable tidal tail or stream extending from the main body. The core region exhibits a concentrated luminosity, possibly indicating a bulge component or active galactic nucleus. Color gradients within the galaxy suggest varying stellar populations and star formation activity. There appears to be some blue tinges within the main body of the galaxy. The shape is elongated and not particularly round.
