The galaxy presents as a single, relatively smooth concentration of light. It appears elliptical in shape, with a high degree of central concentration, lacking any distinct spiral arm structures. The light distribution is fairly uniform across the visible body of the galaxy with what appears to be a slightly brighter core region. No strong dust lanes or prominent star-forming regions are discernible in this image. There is no obvious evidence of tidal features or distortions suggestive of recent major merger activity; only minor disturbances might be present. The galaxy has a yellow-reddish overall hue. The galaxy is likely a massive and relatively passive system with a low star formation rate. 
