The galaxy presents as a generally smooth, elliptical structure with a high degree of central concentration. Its overall color appears slightly redder in the core, transitioning to bluer hues in the outer regions. There is no clear evidence of spiral arms or a prominent disk. The light distribution is centrally dominant, with a gradual decrease in brightness as the radius increases. The galaxy appears slightly elongated. No significant signs of tidal disturbances, major mergers, or active galactic nuclei are immediately apparent from the image.
