The galaxy presents an elliptical morphology with a high degree of central concentration. It appears quite smooth, lacking any obvious spiral arm structures or significant dust lanes. The color gradient suggests a population of older stars, transitioning from yellow-orange in the core to a slightly bluer hue in the outer regions. There's a hint of extended halo surrounding the main body of the galaxy. The shape is close to circular, showing no clear signs of tidal interactions or major disturbances. Based on its appearance, this is likely a relatively massive galaxy with a substantial stellar population.
