The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated bulge that is bright and yellow, suggesting an older stellar population. The overall form of the galaxy is fairly round, showing minimal signs of significant tidal disturbances or ongoing major mergers. There is a faint disk, which appears to be composed of a low amount of dust, and active star formation is present, as is evidenced by the blue hue in the outskirts of the galaxy. 
