The galaxy presents as a smooth, elliptical structure with a bright central bulge. The light distribution suggests a relatively even dispersion of stars throughout the main body, with a concentration of luminosity toward the core. The color profile transitions from a bluer hue at the core to a yellower tone in the outer regions. There is little evidence of spiral arms or significant dust lanes, indicating a lack of active star formation. There is no major interaction or merger events occurring with nearby galaxies.