The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution suggests that the bulge component dominates the overall light profile. There is a subtle color gradient, transitioning from a more yellow-red hue in the central region to slightly bluer colors in the outer regions, which may indicate a decreasing age of the stellar populations further away from the galactic center. The galaxy is generally round in shape. There are no obvious signs of major mergers or significant tidal disturbances in its structure. Overall, the galaxy seems to have low ongoing star formation.
