The galaxy exhibits a morphology that is suggestive of an ongoing merger event. There appears to be a primary galactic core with a companion core in close proximity. The light distribution is relatively smooth, with an overall elliptical shape. Color gradients suggest that the central region is generally composed of older stellar populations, with some evidence of recent or ongoing star formation in the outer regions. This is evidenced by slightly bluer light emitted from the edges of the galaxy. The system's estimated size is approximately 6 kpc.
