The galaxy presents as a relatively smooth, elliptical structure. It appears centrally concentrated with a bright, unresolved nucleus. The luminosity profile decreases gradually from the core outwards, suggesting a lack of distinct spiral arms or other prominent features. The galaxy's shape is mostly round, with a slight deviation towards being slightly less circular. There are no immediately obvious signs of major mergers or significant tidal disturbances, however a minor disturbance cannot be ruled out. Colors suggest an older stellar population. There is little evidence of active star formation within the visible bands, as the galaxy is red and lacks blue knots or HII regions.
