The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. There is no apparent spiral structure or distinct disk. The light distribution is centrally concentrated, fading gradually outwards. The overall color appears relatively uniform with a slightly bluer core region and redder outskirts. This suggests a population of older stars towards the edges and possibly more recent star formation in the core. There are no obvious signs of tidal tails or other major distortions indicative of a recent major merger event, though a slight asymmetry could indicate minor disturbances. The galaxy is moderately bright. Its apparent roundness suggests it's being viewed close to face-on. 
