The galaxy presents a smooth, elliptical morphology with a bright, concentrated central bulge. The overall color appears to be reddish, suggesting an older stellar population with fewer young, massive stars. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a relatively high degree of ellipticity, appearing somewhat flattened. No obvious signs of recent or ongoing mergers or tidal disturbances are visible. The galaxy's light profile is well-defined, and the luminosity distribution follows a smooth decline from the center outwards.
