The galaxy presents as a single, centrally concentrated object with a smooth, elliptical morphology. The light profile appears to be well-defined, exhibiting a gradual decrease in intensity from the core outwards. The core itself displays a yellowish-white hue, which likely indicates an older stellar population. Moving outwards from the center, the color shifts towards a redder tone. There is no discernible disk component or spiral arm structure. There are no distinct tidal features or distortions to suggest any recent major merger activity. The light distribution has a generally rounded shape, with minimal elongation.
