The galaxy presents a relatively smooth morphology. It appears to be largely spheroidal in shape, with a high degree of central concentration. The light distribution is generally even, suggesting an older stellar population. A faint, diffuse halo is seen extending outward from the central region, fading gradually into the background sky. There are no obvious signs of spiral arms or a well-defined disk structure. Subtle color variations are present. The core appears slightly yellower than the outer regions, which have a bluer hue. No signs of active galactic nuclei are apparent.
