The galaxy presents as a centrally concentrated, relatively smooth object with a distinct but not perfectly circular morphology. It displays a general spheroidal shape, possibly leaning towards an elliptical form. There is a noticeable color gradient, with a more yellowish-orange hue towards the center that transitions to a bluer periphery. This could indicate an older stellar population concentrated in the core, with more recent star formation occurring in the outer regions, although the relatively high smoothness fraction suggests the star formation is not occuring in obvious spiral arms. There is some asymmetry to the outer structure, hinting at past interaction with another galaxy or other minor disturbances. Based on the color, stellar mass, and relatively low specific star formation rate, it could be a galaxy transitioning from a more actively star-forming state to a more quiescent phase. The high smoothness fraction suggests that this is likely a very mature galaxy.
