The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high surface brightness with a yellowish-gold hue, suggesting an older stellar population. Moving outward from the center, the galaxy displays a gradual decrease in brightness. There is evidence of some bluer regions, hinting at some star formation activity, likely concentrated in the outer regions. Some subtle disturbances could be present in the galaxy's morphology. The overall shape is somewhere between a perfect sphere and a cigar shape. The galaxy is moderately large and exhibits signs of neither an ongoing merger nor any tidal disturbances, but likely experienced some smaller disturbance event in the recent past.
