The galaxy presents a smooth, elliptical morphology. The central bulge is prominent and displays a yellowish hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a slightly bluer tone, indicating the presence of younger stars in the galactic disc. The overall shape leans towards a flattened spheroid, rather than a perfect sphere. There is no discernible spiral arm structure or distinct dust lane features visible. The galaxy appears relatively undisturbed, showing no obvious signs of recent or ongoing major merger activity, but a minor tidal disturbance cannot be ruled out based on the faint asymmetry in the outer regions of the galaxy.
