The galaxy presents a mostly smooth, elliptical morphology with a bright, concentrated central bulge. The light distribution suggests a relatively high degree of rotational symmetry, although there's a subtle elongation. The galaxy displays a color gradient, with the central region appearing bluer and the outer regions progressively redder. This color variation could indicate differing stellar populations, with younger, bluer stars dominating the center and older, redder stars populating the outskirts. There is evidence of minor disturbances, but no signs of ongoing major mergers.
