The galaxy presents a generally smooth and elliptical morphology. The central region is characterized by a bright, concentrated core exhibiting a yellowish-orange hue, suggestive of an older stellar population. Extending outward from the core, the galaxy displays a less defined, diffuse halo. Faint blue tinges are visible within the outer regions, possibly indicative of more recent star formation, though not pronounced. Overall, the galaxy appears to be relatively undisturbed, showing no signs of a major ongoing merger, although there may be some minor disturbances of the galaxy. The axial ratio indicates that the galaxy is not perfectly circular, but appears somewhat flattened or elliptical.
