The galaxy presents as an elliptical or lenticular type object, exhibiting a largely smooth and centrally concentrated light distribution. The core appears to be a bright yellow color, which could be due to high concentration of older stars and a lack of significant dust obscuration. The isophotes display a roughly circular geometry, showing minimal signs of disk-like structure or tidal disturbances. There is little evidence of recent or ongoing star formation, based on the absence of blue-shifted light. The galaxy doesn't show indications of morphological perturbation, suggesting it is not undergoing any major merger events.