The galaxy presents as a relatively smooth, rounded object, appearing largely undisturbed. The galaxy's color profile suggests an older stellar population, with a dominant yellowish-orange hue indicative of evolved stars. There is no visually discernable spiral structure or pronounced disk component within the galaxy. Subtle color variations may be present, however, the resolution limits detailed analysis. Any structure that may be present is very compact and the outer halo regions fade gradually. There is no apparent active galactic nucleus or quasar at the center. Based on this information, the galaxy is likely to be an elliptical galaxy, without significant amounts of ongoing star formation.
