The galaxy presents a disturbed morphology, suggestive of an ongoing or recent interaction. Its overall shape is elongated and somewhat irregular. There appear to be two distinct, bright central concentrations of light, implying the presence of two galactic nuclei. A fainter, more diffuse stellar population surrounds these nuclei, forming a hazy envelope that extends beyond the bright central regions. There are hints of tidal features or tails emanating from the galaxy, further supporting the interaction scenario. These features are faint and diffuse, suggesting a relatively old or advanced stage of the interaction. The galaxy's color is relatively uniform, without obvious strong color gradients or prominent star-forming regions.
