The galaxy presents as a somewhat elongated, elliptical structure. Its central region exhibits high luminosity, suggesting a significant concentration of stars, likely an older stellar population given the overall color. The outer regions display a gradual decrease in surface brightness, with a faint halo extending along its major axis. There is a slight asymmetry visible, potentially indicative of past or ongoing interactions. Overall, the galaxy appears relatively smooth in texture, with no prominent spiral arms or dust lanes readily apparent in this image. The light appears to be slightly redder towards the center and more blue on the edges, indicative of some differences in the star populations throughout the galaxy.
