The galaxy presents as a centrally concentrated, smooth object with a rounded morphology. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The luminosity decreases radially outwards, fading into a bluer halo or extended envelope. The object appears relatively undisturbed, without significant tidal features or indications of a major merger event. There is a subtle color gradient from the core to the outer regions, transitioning towards slightly bluer tones. The galaxy's overall structure suggests a classification leaning towards an elliptical or lenticular type, with a dominant bulge and minimal signs of spiral arm structure.
