The galaxy appears to be a relatively smooth, elliptical galaxy. Its color gradient transitions from a bright, yellowish-white core to a bluish-tinged outer region. The galaxy exhibits an elongated shape, appearing more oval than circular. There is a slight asymmetry to the galaxy, with a subtle extension towards the right. There is very little visible structure, such as spiral arms or dust lanes. The light distribution indicates a high degree of central concentration, suggesting an older stellar population. Evidence of any major ongoing mergers or significant tidal disturbances is absent, though minor disturbances might be present.
