The galaxy presents a largely smooth and somewhat elliptical morphology. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue suggestive of an older stellar population. Surrounding the core is a more diffuse and fainter halo region. There is some hint of a disk-like structure, but it is not prominently defined. Some minor disturbances or asymmetries may be present in the outer regions, potentially hinting at past minor interactions or mergers, though the main body of the galaxy appears relatively undisturbed. There does not seem to be a high rate of star formation within the galaxy.
