The galaxy presents a morphology dominated by a smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish-white color, indicative of an older stellar population. Surrounding the core, there is a broader, more diffuse greenish halo that suggests the presence of more recent star formation. The overall shape is somewhat elliptical, though not perfectly spherical, leaning towards a more moderately elliptical form. Faint distortions are visible in the outer regions of the galaxy, and a slight asymmetry can be observed. These features hint at possible interactions with another galaxy, though definitive merger features are absent.
