The galaxy presents as a relatively compact and luminous object. Its overall morphology is smooth and elliptical, showing a high degree of central concentration. There is minimal evidence of spiral arms or a distinct disk structure. The galaxy's color is somewhat red, indicative of an older stellar population and a lower rate of on-going star formation. The light is fairly evenly distributed, without significant knots of star formation that would suggest a more active star-forming region. There is a very subtle asymmetry, but nothing to indicate a major merger or tidal interaction. The overall form appears to be closest to an elliptical galaxy with a high degree of sphericity.
