The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a high concentration of luminosity, appearing as a bright, yellowish core. This core gradually fades into the outer regions of the galaxy. The shape approximates a slightly elongated, but mostly round. There is no discernible spiral arm structure or significant dust lane obscuration evident. Overall, the galaxy appears relatively undisturbed, exhibiting no signs of major mergers or tidal interactions. The color profile suggests an older stellar population, typical of elliptical galaxies. The faintness of the outer regions indicates a low rate of recent star formation.
