The galaxy presents a morphology consistent with an elliptical or lenticular type. The central region exhibits a pronounced bulge, characterized by a yellow-orange hue indicative of an older stellar population. The overall light distribution appears relatively smooth, though with subtle irregularities that suggest possible tidal features or internal disturbances. The outer regions display a faint, diffuse halo, with a slight blueish tinge. There are some subtle signs of a disk, but there is no clear spiral arm structure present. The morphology of the galaxy could also be indicative of a past or ongoing merger.
