The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, featureless morphology. The light distribution suggests a generally round shape with a moderate concentration of light toward the center. However, the light distribution is visibly disturbed, and there are multiple distinct light concentrations which appear to be the remnants of mergers. There are also visible disturbances, but are too indistinct to be clearly classified without further observation. The overall color appears to be on the redder end of the spectrum, suggesting an older stellar population.
