The galaxy presents as a relatively smooth, elliptical-like structure. The light profile appears concentrated towards the center, suggesting an older stellar population. There is a slight elongation, however the galaxy is mostly round. There are no discernible spiral arms or prominent dust lanes within the visual data. There is evidence of disturbances in the galaxy, with slight variations in color temperature across the surface of the galaxy. The overall color suggests a population of older stars, however a small amount of star formation cannot be ruled out. It is possible the galaxy is in the process of merging with another galaxy. 
