The galaxy presents a relatively smooth, concentrated morphology. It exhibits a primarily elliptical shape, appearing mostly round with slight deviations toward an intermediate form. The galaxy displays a central bulge that appears bright and yellowish in color, suggesting a population of older stars. The outer regions of the galaxy fade into a less defined halo, showing a subtle blue tint indicating the presence of younger stellar populations, although the overall star formation activity seems to be low. There is no apparent evidence of strong tidal disturbances or recent major mergers in its overall form, though minor asymmetries could suggest past interactions.
