The galaxy presents an elliptical morphology. It exhibits a smooth light distribution across its visible extent with no apparent spiral arm structures. The color gradient suggests an older stellar population with a reddish hue dominating the galaxy's body.

There is a notable presence of a potential merger. Two bright areas are embedded in the center, which could be either distinct nuclei, or simply areas of extremely high concentrations of stars. These areas appear closely connected to each other.

The overall structure of the galaxy appears disturbed, possibly due to tidal forces exerted during the merger process. Faint extensions of material extend on either side of the galaxy. A significant portion of the light comes from this central merging region.
