The galaxy presents as a single, moderately luminous object with a smooth, elliptical morphology. There is a high degree of central concentration as evidenced by the bright nucleus. Proceeding outwards, the light intensity gradually decreases to a diffuse halo. Color gradients are subtle, with a tendency towards redder hues in the outskirts. No distinct spiral arms or bar features are observed. Minor asymmetry is possible as hinted by the overall shape of the galaxy. Overall, the galaxy appears to be in a relatively quiescent state, with little evidence of ongoing major star formation or active galactic nucleus activity.
