The galaxy presents a largely smooth, elliptical morphology with minimal discernible structure. It appears nearly round. A bright, concentrated core dominates the galaxy's center, indicating a potentially high stellar density in the central region. Moving outward from the core, the light gradually fades, revealing a diffuse halo. The galaxy exhibits a color gradient, with the central region appearing more yellow, possibly due to an older stellar population. The outer regions are less red, suggesting a slightly younger population. There is no obvious indication of spiral arms, bars, or major disturbances from interactions with other galaxies. The overall color and smoothness suggest an evolved system with a low rate of star formation.
