This galaxy appears to be a relatively smooth, elliptical galaxy. Its central region exhibits a high concentration of light, suggesting a dense stellar population, while the outer regions show a gradual decrease in luminosity, indicative of a decreasing stellar density with increasing radial distance. The overall color of the galaxy is slightly blue, which could indicate the presence of a small amount of ongoing star formation. There are no discernible spiral arms or prominent dust lanes evident in the image. The galaxy appears quite round, with no significant elongation or signs of major tidal disturbances. The galaxy appears as a singular object with no noticeable merger features.
