The galaxy appears to be a relatively smooth, elliptical galaxy. Its light profile suggests a high degree of radial symmetry. The galaxy exhibits a central concentration of light, appearing brightest in its core, with a gradual decrease in luminosity outwards. There is a subtle color gradient with the core appearing yellower and the outer regions slightly redder, suggesting a possible difference in stellar population age and metallicity between the galaxy's nucleus and its surrounding regions. There is no noticeable disk component or spiral arm structure visible in the image. The overall morphology indicates a relaxed system with no apparent major disturbances or ongoing merger activity.