The galaxy presents a generally smooth and rounded morphology. There is a concentration of light in the center. The galaxy has a near spherical shape. Based on the color distribution, the galaxy has a relatively old stellar population and low star formation rate. There is no evidence of spiral arms or a disk-like structure, nor any signs of major mergers or tidal disturbances, such as plumes or tails. There may be some minor interaction with a neighboring object, but that is hard to tell from this image. 
