The galaxy presents a complex morphology, potentially indicating an ongoing or recent interaction. The primary structure appears elongated and somewhat irregular, suggesting a disturbed disk or tidal features. A distinct, brighter region, possibly a galactic nucleus or a region of intense star formation, is visible at one end of the elongated structure. There is a noticeable color gradient across the galaxy, with bluer hues dominating in the brighter region and extending along one side of the elongated structure, indicative of younger stellar populations. Fainter, diffuse extensions or tidal tails are observed, further supporting the hypothesis of gravitational interaction or a merger event. A slight reddish region is near the middle of the galaxy. Overall, the galaxy exhibits signs of dynamical activity and complex stellar populations.
