The galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated. The light distribution suggests a higher density of stars towards the core, gradually decreasing outwards. There is a slight elongation along one axis but generally, its shape is more rounded. No distinct spiral arm structures are apparent in this image. There is a hint of blue suggesting a small component of young stars. The overall color is consistent with an older stellar population. There is no obvious evidence of significant ongoing mergers or major disturbances.
