The galaxy presents a largely smooth morphology, exhibiting a significant central bulge. The object is substantially rounded with only a slight deviation from circular symmetry. There is an apparent absence of spiral arms or a well-defined disk structure. Indications of past or ongoing merger activity appear to be minimal, with no obvious tidal tails or significant morphological disturbances. The object displays a color gradient, transitioning from a yellowish central region to a bluer halo, which implies radial variation in stellar populations or dust content.
