The galaxy presents a complex morphology, appearing as an ongoing merger of multiple components. The primary body exhibits a relatively smooth, elliptical profile. Evident in the system are significant tidal features, with disrupted structure indicative of gravitational interactions.

One component displays a bluer hue, potentially signifying younger stellar populations and ongoing star formation activity. Conversely, another area is characterized by a reddish tint, likely indicative of older, cooler stellar populations. The galaxy is intermediate in shape. Based on the evidence, it appears to be undergoing a significant period of morphological transformation, resulting in widespread disruption.
