The galaxy exhibits an elliptical morphology, with a smooth, centralized concentration of light. The color profile is generally redder, suggesting an older stellar population. There may be minor irregularities in the light distribution suggesting some kind of minor disturbance. It displays an apparently high Sersic index, indicating it is most likely an elliptical or lenticular galaxy. There is also a possibility that this could be an ongoing or recent merger between 2 galaxies. 
