The galaxy appears as a relatively smooth, elliptical-shaped object. Its color is generally consistent across its structure, displaying a slightly yellowish hue. There may be a subtle central concentration of light, but the gradient is quite shallow. There are no clear signs of spiral arms or a distinct disk, and the galaxy appears to be quite round. There is no evidence of ongoing major mergers or significant tidal disturbances. Based on its morphology and color, this galaxy likely consists primarily of older stellar populations with a low rate of star formation.
