The galaxy appears to be a luminous, relatively smooth elliptical galaxy. It has a concentrated central bulge with a decreasing luminosity gradient outward. The core is a yellowish hue, suggesting an older stellar population. The outer regions exhibit bluer tints, which might imply a younger population of stars in the outskirts of the galaxy, although the overall smooth texture would imply these are not major star-forming regions or spiral arms. There are no obvious signs of strong tidal disturbances or a major ongoing merger. It appears to be a fairly relaxed, though not perfectly spherical, system. There are faint indications of some minor structures or irregularities around the main body, but it is difficult to ascertain their nature.
