The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high surface brightness, appearing a golden hue, likely indicating a concentration of older stellar populations. There's a gradual decrease in luminosity moving outward from the core, with the outer regions appearing more diffuse and reddish. No distinct spiral arm structures or prominent dust lanes are discernible. The overall structure indicates a relaxed system with little ongoing major merging activity. There may be minor disturbances or tidal features present but the resolution of the image limits further analysis. The galaxy is generally round in shape.
