The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The color gradient suggests a population of older stars, with a yellowish hue dominating the core region. There is a subtle decrease in intensity from the center outwards, characteristic of a spheroidal stellar distribution. The lack of prominent spiral arms or dust lanes further reinforces the classification as an elliptical galaxy. The object exhibits a high degree of roundness in its overall shape. There are no apparent signs of major ongoing mergers or significant tidal disturbances in this image.
