This galaxy exhibits a primarily smooth morphology, with a slight deviation from a perfectly circular shape. The galaxy appears somewhat flattened or elliptical, with its light distribution concentrated toward the center, suggesting a bulge component. There's a subtle hint of a disk-like structure, but it is not prominently defined. The light profile appears relatively uniform and diffuse, possibly indicating a lack of significant ongoing star formation, or a more distributed pattern of star formation throughout the galactic body. There is no prominent tidal features or signs of major mergers. The galaxy is not strongly elongated. The observed color suggests it is composed of older stellar populations.
