The galaxy presents as a relatively compact, elliptical morphology. Its light profile appears smooth and centrally concentrated, with a noticeable decrease in luminosity towards the outer edges. The color indices suggest a population of older stars, with a dominant yellowish-red hue, indicative of lower star formation activity. There may be evidence of a slight disturbance, with a hint of tidal features that suggests it may have undergone a minor interaction with another galaxy in the past. There is a faint diffuse halo surrounding the central body of the galaxy. The galaxy exhibits a notable degree of roundness.
