The galaxy appears to be undergoing a merger. The system is dominated by two primary components. One component is characterized by a smooth, elliptical morphology. Its core is bright with a relatively even distribution of light.

The second component exhibits a more irregular shape, with some indication of disk-like structures. The color suggests the presence of older stellar populations. Tidal features are not clearly defined, but there might be a faint bridge of material connecting the two galaxies. Overall, the system's morphology indicates a late-stage merger event, where the individual components are not yet fully integrated. Star formation is low.
