The galaxy appears to be undergoing a significant merger event. Morphologically, it presents with characteristics of multiple interacting galaxies. There are three distinct light concentrations, the two brighter appearing to be at the core of each galaxy, and the third more diffuse.

The overall color profile suggests a population of older stars, with a tendency towards the redder end of the spectrum. The image data hints at a relatively low rate of on-going star formation. The main body of the galaxy displays a mostly smooth texture, with the exception of the merging components and some minor disturbances. The galaxy is more elongated than circular.
