The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a centrally concentrated light profile. The color is predominantly yellowish-orange, suggesting an older stellar population with a low rate of current star formation. There is little evidence of spiral arms or significant dust lanes. The galaxy is not perfectly spherical, showing a slight elongation. There are no obvious signs of any major interactions or mergers with other galaxies, though a minor disturbance cannot be ruled out.
