This galaxy exhibits a smooth, elliptical morphology. It displays a concentrated central bulge, characterized by a yellowish hue indicative of an older stellar population. There is little evidence of spiral arms or significant dust lanes within the galactic disk. The galaxy's overall shape appears relatively round, with no major disturbances or signs of ongoing mergers readily apparent. The color profile suggests that star formation activity is likely low within the galaxy. The galaxy's moderate size suggests a substantial stellar mass. 
