The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that gradually diffuses outwards. The galaxy shows a yellow-red hue, possibly suggesting an older stellar population with less active star formation within the galactic disk. It appears quite rounded, showing no strong indication of spiral arms or a disk structure. There are no obvious signs of any recent or ongoing major mergers or tidal disturbances in the galaxy's shape. Based on its visual characteristics, this galaxy is likely to be massive.