The galaxy appears to be a generally smooth object, with a centrally concentrated luminosity profile. A slight elongation in the shape of the galaxy is observed, suggesting a possible ellipsoidal morphology, but it is very close to spherical. The central region of the galaxy is significantly brighter than the outer regions. The color is generally uniform, indicating that the stellar population is relatively well-mixed. However, a faint ring-like structure is potentially present, suggesting past interactions with other celestial objects, but requires further investigation. There do not appear to be any major distortions in its morphology, such as tidal tails or obvious signs of recent merger activity. The light from the galaxy is spread across a small angular area.
