The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, with a dominant bulge component and little evidence of spiral arms or a prominent disk. The light profile shows a gradual decrease in intensity from the center outwards. The color is slightly bluer toward the center. There may be some evidence of minor disturbance in the outer regions of the galaxy, but it appears relatively isolated, not undergoing any major merger events.
