The galaxy presents as a relatively compact, elliptical-like structure with a smooth, diffuse appearance. The light is concentrated toward the center, indicating a dense galactic nucleus. The overall color of the galaxy appears to be yellowish-orange, suggesting an older stellar population with fewer young, massive blue stars. There is little evidence of spiral arms or significant dust lanes. A slight elongation is observed, deviating from a perfect sphere. No tidal tails or obvious signs of a major ongoing merger are readily apparent, though subtle disturbances cannot be ruled out. The galaxy appears relatively isolated.
