The galaxy appears to be a relatively smooth, elliptical type. It has a concentrated central bulge with a moderate halo. The shape is mostly in between round and cigar shaped with an appearance of a smooth object rather than a spiral galaxy. There is a slight indication of a possible minor disturbance in the outer regions and no obvious sign of any merging activity. Based on color, the galaxy appears to be mostly composed of older stars, with a lower star formation rate.
