This galaxy presents as a relatively compact and luminous object. Its morphology appears largely spheroidal, with a smooth, centrally concentrated light distribution. The galaxy exhibits a dominant bulge component with minimal visible disk structure. There is a subtle color gradient, appearing slightly bluer in the inner regions and redder towards the outer halo. Indications suggest ongoing, though perhaps relatively subdued, star formation activity within the galaxy. No obvious signs of major mergers or tidal disturbances are visible. The galaxy is moderately massive. Based on its observed features, this is likely an elliptical galaxy.
