The object appears to be a merging system, likely composed of two galaxies in close proximity. The individual galaxies exhibit a smooth morphology, appearing elliptical in shape with no obvious spiral arm structures. They are generally rounded but slightly elongated along the axis connecting the two objects, suggesting a possible tidal interaction. The color of each galaxy is predominantly yellow-orange, indicating a population of older stars and a low rate of star formation. There is some evidence of a possible minor disturbance in the overall structure, possibly caused by the gravitational interaction between the two galaxies. The overall impression is of a system undergoing a merger event, with the component galaxies in the later stages of the process, possibly coalescing into a single, more massive elliptical galaxy.
