The galaxy exhibits a somewhat disturbed morphology. The central region appears relatively smooth, transitioning outward to a more irregular structure. There is a faint suggestion of a disk component, but it is not well-defined. There's possible minor asymmetry, but the overall shape appears roughly elliptical. The galaxy exhibits color variation, appearing bluer towards the central region and redder further out. This color difference may indicate a difference in the stellar populations and star formation rates between the center and the outer regions of the galaxy. There may be some evidence of tidal features, perhaps a faint stellar stream or distortion hinting at gravitational interaction with another galaxy.
