The galaxy presents as a relatively smooth, centrally concentrated structure. Its overall form appears elliptical, with a diffuse halo extending outwards. The core region exhibits a bright, yellowish-orange hue, suggesting a population of older stars. There is a subtle gradient in color towards the outer regions, with a slightly bluer tint indicating the presence of younger stars in the surrounding area. The galaxy does not show strong evidence of spiral arms or significant disk features. However, there are subtle irregularities within the halo, which may indicate minor disturbances. Based on the brightness and color indices, the galaxy is likely a massive system with a moderate rate of star formation. It seems to be either undergoing or to have recently undergone a merging event that is still subtly disturbing its structure. 
