The galaxy appears to be an elliptical or lenticular type. It exhibits a generally smooth, centrally concentrated luminosity profile, with the light gradually fading towards the outer regions. The color is predominantly yellow-orange, suggesting an older stellar population with a relatively low rate of recent star formation. There may be a slight indication of a disk-like structure, but this is not definitive. Overall, the galaxy appears relatively undisturbed, showing no clear signs of major merger activity, though minor disturbances can't be ruled out.
