The galaxy presents a largely smooth and rounded morphology. A concentrated central bulge is evident, exhibiting a bright, almost stellar-like core. Surrounding the core, the galaxy appears to have a diffuse halo. There is a subtle suggestion of spiral structure or perhaps a disk component, but it's not prominent, potentially due to the galaxy's inclination or inherent structure. The color gradient suggests that the core and central region are bluer than the outer regions, which tend towards redder hues. This may indicate differing stellar populations or dust content. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There may be minor disturbances present, but this is not entirely clear.
