The galaxy appears as a single, dominant, and relatively smooth light source. It exhibits a concentrated, elliptical morphology. Its color is predominantly yellow, suggesting an older stellar population and potentially a lower rate of star formation. There is a noticeable lack of spiral arms or any distinct disk features. The overall structure suggests a spheroid-dominated system with a high degree of radial symmetry. No obvious tidal features or signs of recent major mergers are visible. It is an isolated elliptical galaxy.
