The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. It appears relatively undisturbed, showing no clear evidence of ongoing major mergers or tidal disruptions. The light distribution suggests a fairly homogeneous stellar population, with a gradual decrease in surface brightness from the core outwards. There's a hint of color gradient, with the central region perhaps appearing slightly redder than the outer halo, suggesting older stellar populations are more concentrated toward the center. Star formation activity appears to be minimal within the galaxy. Overall, it has the characteristics of a mature elliptical galaxy.
