The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its shape is predominantly elliptical, appearing somewhat elongated rather than perfectly circular. The central region displays a yellowish-white hue, potentially indicative of an older stellar population dominating the core. The outer regions exhibit a faint disk, with a subtle bluish tint suggesting the presence of younger, hotter stars in the disk component. Overall, the galaxy exhibits no major disturbances or prominent tidal features, suggesting it is relatively undisturbed and not undergoing any major merger events. However, there is a slight asymmetry in the outer regions, hinting at the possibility of minor interactions or past disturbances.
