The galaxy appears as a centrally concentrated, elliptical structure with a smooth, relatively featureless morphology. The dominant color is a yellow-orange hue, suggesting a stellar population dominated by older, redder stars with minimal ongoing star formation. The galaxy exhibits a high degree of central light concentration, with a gradual decrease in brightness toward its outer regions. There is a hint of extended diffuse light surrounding the core. No spiral arms or distinct dust lanes are visible. It appears fairly isolated, showing no obvious signs of tidal interaction or ongoing merger activity, although there is minor asymmetry. Its apparent shape appears fairly round.
