The galaxy appears to be a relatively compact, somewhat elliptical object with a smooth, diffuse light profile. Its central region exhibits a higher surface brightness, suggesting a concentration of older stellar populations. A faint disk may be present, but it is difficult to ascertain details with certainty, and the overall morphology appears more spheroidal than spiral. The color suggests that star formation is suppressed. There may be some evidence of a minor gravitational disturbance in the outer regions.
