The galaxy appears to be an elliptical galaxy with a smooth, relatively featureless structure. Its shape is close to circular, exhibiting a high degree of central concentration. The galaxy appears to be largely devoid of spiral arms or significant dust lanes. The color profile suggests an aging stellar population, with a relatively weak star formation rate, which is consistent with a well-established elliptical galaxy. There may be a slight central brightening in the galactic core. There is no evidence of ongoing merger activity or significant tidal disturbances based on this image.
