The galaxy appears to be a relatively smooth, elliptical-like system. Its light is concentrated towards the center, indicating the presence of an old stellar population. The color index indicates a slight red shift which points to the presence of older stars and a diminished rate of star formation. There is a slight deviation from perfect circularity. There is no evidence of prominent spiral arms or a central bar. The morphology suggests that the system is dynamically relaxed. There is no evidence for on going mergers or tidal interactions.
