The galaxy presents a complex morphology, appearing to be in the late stages of a merger event. The dominant feature is an elongated structure with two distinct color gradients. The northern region displays a yellowish-orange hue, potentially indicative of an older stellar population. In contrast, the southern region exhibits a bluer tint, suggesting more recent or ongoing star formation.

There is some evidence of tidal tails, further supporting the merger hypothesis. The galaxy appears to be relatively massive, given its luminosity and the apparent spatial extent of its disturbed morphology.
