The galaxy presents a largely smooth, elliptical morphology. The central region exhibits high luminosity, appearing almost uniformly bright, with a yellowish-white hue. The light intensity decreases gradually outwards from the center, forming a diffuse halo that transitions into the background sky. There is minimal evidence of spiral arm structure or distinct dust lanes, suggesting an older stellar population. The galaxy appears nearly circular, with no significant elongation or tidal distortions visible. Overall, it appears to be a mature, quiescent galaxy. 
