The galaxy presents as an elliptical structure, though with some hints of a disk component. Its overall color is a pale blue, suggesting the presence of a moderate population of younger, hotter stars. There is a bright central region indicative of a galactic bulge or an active galactic nucleus. Some subtle structural features are visible, potentially minor distortions in the galaxy's shape which may be the result of a minor interaction, recent merger, or internal dynamics. The galaxy is relatively compact. The smoothness of the light distribution suggests a somewhat evolved system, but the blue color suggests ongoing star formation.
