The galaxy presents a morphology suggestive of an elliptical or lenticular type. It exhibits a centrally concentrated, smooth light distribution. The core displays a yellowish hue, potentially indicating an older stellar population. Fainter, diffuse extensions are visible around the central region. These outer regions appear less structured, fading gradually into the background. There is a slight asymmetry in the outer light distribution, with a subtle elongation along one axis. No distinct spiral arms or dust lanes are readily apparent. The overall appearance suggests a galaxy that is relatively evolved, with a high degree of internal order and limited ongoing star formation. There are some faint blueish spots in the outer regions, that could signal more recent star formation activity in that region.
