The galaxy presents an elliptical morphology, appearing mostly smooth with a high degree of central concentration. A bright nucleus dominates the structure, fading outwards into a diffuse halo. The isophotes appear somewhat elongated but overall, the galaxy is relatively round. There's a hint of a disk-like structure, though not strongly defined. Based on the galaxy's color and the observed star formation rate, the galaxy's stellar population likely consists of older stars with little to no on-going significant star formation. There is the possibility of a minor disturbance in the outer regions, which could indicate a past or ongoing minor merger event. Overall, the galaxy appears to be a relatively quiescent system.
