The galaxy presents as an elliptical or lenticular type. It displays a smooth, somewhat rounded morphology, with a central bulge that appears slightly elongated. The core of the galaxy exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the core, a faint disk is suggested by the extended but diffuse blueish glow, indicating the presence of some younger stars or star formation regions. However, this disk is not clearly defined, the galaxy appears relatively undisturbed. There is no clear evidence of a major ongoing merger, although there are some minor asymmetries, possibly indicating minor gravitational disturbances or past interactions. The overall structure suggests that the galaxy is relatively evolved.
