The galaxy presents a predominantly smooth morphology, exhibiting minimal discernible features such as spiral arms or a prominent disk structure. It appears approximately round in shape, with a color gradient transitioning from a yellowish core to a bluer halo. The central region is significantly brighter and more concentrated, suggesting a high stellar density, potentially indicating an older stellar population dominating the core. The outer regions are less defined, fading into the background sky. There is no apparent evidence of ongoing major mergers or significant tidal disturbances. Overall, the galaxy seems to be an elliptical galaxy or a lenticular galaxy seen face-on.
