The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The overall shape is mostly round. There's a subtle color gradient noticeable, shifting from a yellowish-white hue in the core to a slightly bluer tint in the extended halo. There is no evidence of prominent spiral arms or significant dust lanes, suggesting it is a mature system with a relatively quiescent star formation rate. No signs of tidal disturbances or ongoing mergers are immediately apparent, implying the galaxy is relatively undisturbed.
