The galaxy presents as a relatively smooth, centrally concentrated structure. Its overall shape is elliptical, appearing quite round. The light distribution suggests a fairly uniform stellar population with a dominant bulge component. There is a subtle hint of extended material surrounding the central region that seems to be a faint halo or disk. The galaxy's color is slightly on the redder side, which would be consistent with an older stellar population and possibly a low rate of star formation. There appears to be very slight evidence of a minor disturbance.
