The galaxy presents an overall elliptical morphology, appearing largely smooth and centrally concentrated. The core exhibits a yellowish hue, suggesting an older stellar population. Moving outwards, the color shifts toward a slightly bluer tone, particularly in the outer regions, possibly indicating regions of more recent, albeit subdued, star formation. Subtle asymmetries are apparent within the main body of the galaxy, suggesting minor gravitational interactions or disturbances. These disturbances could also be caused by minor interactions with smaller satellite galaxies. There is no clear evidence of spiral arm structure or a prominent disk. The galaxy appears relatively undisturbed with no large merger events.