The galaxy appears to be a pair of interacting galaxies. The larger galaxy presents as a relatively smooth, elliptical system with a bright, concentrated central bulge. It exhibits a yellowish-white hue, suggesting an older stellar population with a decreased rate of star formation. It seems that the shape is close to an elliptical structure. The other galaxy has a disk-like component to it, but also has a central bulge. It is a yellowish-white hue similar to the larger galaxy, indicating a similar stellar population. There is a likely merger event between the galaxies that is only subtly distorting the structure, and it is possible it will merge to form a larger elliptical galaxy. 
