The galaxy appears as a single, relatively smooth concentration of light. It exhibits a roughly elliptical morphology, showing a high degree of central concentration, with a slightly diffuse halo surrounding the central region. The core is a yellowish-orange hue, perhaps indicating an older stellar population. The outer regions display a faint greenish tint which could be due to younger stars. There is no strong evidence of spiral arm structure or significant dust lanes. The overall structure suggests an evolved galaxy, likely an elliptical or lenticular type, and shows little evidence of ongoing major mergers or tidal disturbances.
