The galaxy exhibits a largely smooth morphology, suggesting it is likely an elliptical or lenticular galaxy. There's a slight elongation, but overall it appears relatively round in shape. The light distribution is concentrated towards the center, fading gradually outwards. The color profile is relatively uniform, with a reddish hue, which could indicate an older stellar population with less ongoing star formation. There is a small possibility that there are minor disturbances or subtle features implying that the galaxy could have experienced minor merging events in the past.
