The galaxy presents a somewhat irregular morphology. A dominant, relatively smooth central region is observed, though it is not perfectly symmetrical. Fainter, more diffuse structures extend outward from this central area, suggestive of tidal features or disrupted arms. These features are characterized by a bluer color compared to the core, possibly indicating regions of recent or ongoing star formation. There is evidence of disturbance in the galaxy's structure, likely a minor or major merger, but not a complete merger. The galaxy appears to be in the early stages of development.
