The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that appears bright and yellowish-orange, likely indicative of an older stellar population. The outer regions of the galaxy are less defined, fading into the background sky, and show some evidence of a faint greenish hue which may represent younger stars or nebulae. The overall shape appears to be largely spheroidal, with only a slight deviation from perfect roundness. There are no obvious signs of a major ongoing merger or tidal disturbances.
