The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that is yellow-orange in color, suggesting an older stellar population. The outer regions appear less defined and somewhat elongated, possibly indicating a disk-like structure viewed at an angle, but lacking distinct spiral arms. There is no obvious sign of strong ongoing star formation, with the galaxy instead appearing largely quiescent. Faint blue hints in the outer edges could suggest some recent, limited star formation activity. No significant tidal features or signs of an ongoing merger event are apparent. The galaxy presents a generally undisturbed morphology.
