The galaxy presents a largely smooth, elliptical morphology. Its overall color index suggests a relatively evolved stellar population, with a dominant yellowish-orange hue. The light is centrally concentrated, exhibiting a gradual decrease in surface brightness outward from the core. There is a possible subtle disk component, but no spiral arms or prominent star-forming regions are discernible. There is no evidence of major mergers or significant tidal disturbances in the immediate vicinity. The galaxy appears nearly round in projection, showing minimal elongation.
