The galaxy presents an overall elliptical morphology. The central region exhibits a bright, yellowish hue, suggesting a significant population of older stars. Surrounding the central bulge, there is a more diffuse, greenish component, possibly indicative of more recent star formation or ionized gas. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal features. There is a slight asymmetry in the distribution of the greenish component, with a more pronounced presence towards the upper portion of the galaxy. The outer regions fade gradually into the background, with a smooth transition in color and luminosity. The color profile suggests that the galaxy is relatively evolved, with a moderate amount of on-going star formation.