The galaxy appears as a well-defined, centrally concentrated object with a smooth morphology. Its overall shape is elliptical, displaying a high degree of roundness with a slight deviation towards an intermediate form. There are no readily apparent signs of spiral arms or a disk structure. The galaxy exhibits a color gradient, transitioning from a bluer core to redder outer regions. No significant indications of ongoing merging events or major disturbances are observed in the galactic structure. The absence of prominent features suggests a relatively evolved system, potentially with a stabilized morphology.
