The galaxy presents a largely smooth morphology, with a highly concentrated central bulge. The color gradient transitions from a yellow-white core to a bluish outer halo, potentially indicating a mix of older stellar populations in the center and younger, bluer stars towards the periphery. The galaxy appears elliptical or lenticular in shape, lacking any pronounced spiral arm structures or significant dust lanes. There are some very faint signs of disturbances, like a possible very slight tidal tail or faint merging event, but mostly none. Overall, it gives the impression of a relatively evolved system, likely undergoing a relatively low rate of star formation. The galaxy's round shape suggests it likely does not have a disk. 
