The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. There is some evidence of a slight disky feature but it is unclear, and only a minor component of the galaxy's structure. The galaxy has a relatively consistent colour gradient, transitioning from a yellowish hue in the core to slightly bluer tones in the outer regions. There's no obvious evidence of spiral arms or active star formation regions. The overall structure suggests an evolved system, likely comprised predominantly of older stellar populations. There are no major disturbances or signs of recent merger activity visible.
