The galaxy presents as a relatively smooth, luminous object with a high degree of circularity. The light distribution is centrally concentrated with a gradual decline in intensity towards the outer regions. There is a slight asymmetry to the galaxy's outer profile, but it appears to be a largely undisturbed system. Based on the light distribution, a likely classification would be an elliptical or lenticular galaxy. The object has a noticeable blue-green hue, indicating ongoing star formation activity. It is unlikely to be undergoing any major mergers, though minor disturbances cannot be ruled out.
