The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. The core exhibits a strong luminosity, appearing a warm yellowish-orange hue. This could indicate an older stellar population dominating the central region. The outer regions of the galaxy show a gradual decrease in surface brightness. There is a subtle extension of the galaxy's light along what appears to be the major axis, but it is not well defined. Some minor perturbations are potentially visible in the outskirts of the galaxy, suggesting the possibility of tidal interactions or a recent minor merger event, but the central bulk of the galaxy appears relatively undisturbed. Overall, the galaxy appears to be a relatively massive and evolved system.
