The galaxy presents a mostly smooth morphology, with a hint of a flattened, disk-like structure. It appears primarily elliptical in shape, with an aspect ratio suggesting it is viewed nearly edge-on. The central region exhibits a yellowish hue, possibly indicating an older stellar population. Faint blue-ish components appear within it, implying a low level of ongoing star formation. Overall, the galaxy shows no obvious signs of major disturbances or ongoing merger events. There is a subtle suggestion of faint arms or spiral features embedded within the disk. 
