The galaxy appears to be a relatively smooth elliptical galaxy. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The overall color profile suggests an older stellar population, with a yellow-red hue dominating. There's no strong evidence of active star formation regions or distinct spiral arm structures. The galaxy's shape is generally round, without significant distortions or tidal features suggesting recent major merger events. Subtle irregularities may be present, indicating minor gravitational interactions.
