The galaxy presents a largely smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, with light distribution decreasing radially outward. The shape approximates a spheroid with a slight deviation from perfect roundness. No distinct spiral arms or significant dust lanes are apparent. The color profile indicates a bias towards redder hues, particularly concentrated at the center. There is no obvious signs of ongoing major merger events or significant tidal disturbances. The galaxy is likely an evolved system with a relatively low rate of star formation.
