The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a high degree of central concentration with decreasing luminosity towards its outer regions. The central region appears bright, possibly indicating a significant stellar population or active galactic nucleus. The galaxy's overall color appears somewhat blue-white, suggesting the presence of a population of younger, hotter stars, even as its smooth morphology indicates an older galaxy. There is no strong evidence of spiral arms or significant dust lanes. There are no indications of recent major merger activity or tidal disturbances, although there may be minor disturbances or other forms of gravitational interactions present. The galaxy exhibits a circular, smooth appearance. 
