The galaxy presents as a relatively smooth, centrally concentrated structure, likely an elliptical or S0 galaxy. The light distribution indicates a bulge-dominated morphology, with a bright nucleus fading outwards. The galaxy appears to be generally rounded in shape. There is no obvious evidence of spiral arms or distinct features indicative of recent major mergers. The color appears to be a relatively uniform blue, which may suggest that the galaxy is not completely devoid of young stars, although star formation may be at low levels. There is no obvious dust lane or any major distortions in the galaxy's structure, although there are very minor disturbances.
