The galaxy appears to be a relatively smooth, elliptical-type galaxy, displaying a prominent central bulge. The light distribution appears concentrated towards the center, which suggest an older stellar population. Fainter, bluer regions are present in the outer regions. The overall color gradient transitions from a more yellow hue in the central region to slightly bluer hues further from the center, suggesting that star formation may be occurring at low levels. There are no obvious signs of spiral arms or a distinct disk structure. There is some evidence of minor disturbances from the surrounding environment. The galaxy is elongated in shape, but not so much as to be considered cigar-shaped. 
