The galaxy appears to be a luminous, relatively smooth elliptical or lenticular galaxy, likely at an intermediate redshift. The primary body of the galaxy exhibits a concentrated central bulge that dominates the light profile. The galaxy appears somewhat rounded in overall shape, with a subtle elongation suggesting a mild departure from perfect circularity. There is a faint bluish region on one side of the bulge, potentially indicating an area of recent, albeit limited, star formation. The galaxy appears to have undergone minimal disturbance, showing no clear signs of ongoing major mergers or strong tidal interactions. The orange hue indicates a population of older stars.
