The galaxy presents as a luminous, ellipsoidal structure. The central region exhibits a concentrated, bright core that gradually diffuses outward. A smooth, almost featureless morphology is evident, with a high degree of central concentration. There's a subtle color gradient, transitioning from a somewhat bluer hue in the outer regions to a slightly redder tint towards the core. No apparent spiral arm structures or distinct dust lanes are discernible. There is no obvious indication of active merging or major gravitational disturbance from the image. The overall appearance suggests a relatively evolved system dominated by an older stellar population.
