The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing as a concentrated, bright core. This core gradually diffuses outward into a less dense halo. The color profile of the galaxy indicates a dominance of older stellar populations, with a yellowish-red hue most prominent throughout. There is no evidence of distinct spiral arm structures or significant dust lanes within the visible spectrum. The overall shape appears nearly circular and without any signs of major disturbances.
