The galaxy presents an elliptical morphology, appearing largely smooth and rounded in shape. There is a concentration of light towards the center, with a gradual decrease in brightness moving outward. The galaxy exhibits a color gradient, shifting from a yellowish-white core to a slightly redder hue in its outer regions. The galaxy does not appear to be undergoing any major mergers or disturbances, although minor disturbances are possible given the overall appearance. The light distribution suggests a relatively even density of stars, lacking prominent spiral arms or distinct features beyond the central bulge.
