The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. The color profile suggests a dominant older stellar population, with a slight bluer hue in the outer regions. The isophotes appear largely regular with no obvious signs of strong tidal disturbances or ongoing major mergers, though there are some very slight indications of minor asymmetries. The overall morphology is fairly featureless, lacking prominent spiral arms or a distinct dust lane. The galaxy's shape is generally round.
