The galaxy presents as a relatively smooth, elliptical-like object with a high degree of central concentration of light. The core appears bright and yellowish-white, suggesting a population of older stars. The outer regions exhibit a gradual fading of luminosity, with a slight reddish hue. The galaxy appears quite symmetrical, displaying no obvious spiral arm structures or signs of major disturbances. The light distribution is relatively uniform. Overall, the visual impression is that of a mature galaxy with little ongoing star formation.
