The galaxy appears to be a luminous, elliptical or lenticular galaxy with a smooth and concentrated light profile. It presents a predominantly yellow-orange hue, potentially indicating an older stellar population with reduced ongoing star formation. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy exhibits a largely uniform, spheroidal shape, showing high degree of central concentration. There are no signs of major disturbances to its morphology, suggesting the absence of ongoing or recent major merger events. Faint extensions of light surround the main body of the galaxy, which may be indicative of a extended stellar halo.
