The galaxy presents as a moderately luminous, relatively smooth and concentrated elliptical galaxy. Its core exhibits a strong, yellow-white luminosity, suggesting a substantial population of older stars. The overall shape is generally round. The gradient of light intensity decreases smoothly from the center outwards, with no distinct spiral arm structure or prominent dust lanes visible. A faint bluish halo surrounds the central region, possibly indicative of some younger stellar populations or ongoing, but low-level star formation. There is no strong evidence of any major recent or ongoing merger activity within the galaxy, although there are some minor disturbances potentially. Overall, the morphology suggests a galaxy that has largely settled into a stable configuration, with the majority of star formation having ceased.
