The galaxy presents as a single, relatively smooth object, appearing mostly undisturbed. The morphology is generally elliptical, with a high degree of central concentration. The core exhibits a yellow-orange hue suggesting an older stellar population, while the outer regions transition to a bluer color, indicating the potential presence of younger stars. The galaxy's overall shape is moderately rounded, with no obvious spiral arms or bar structures. There are no signs of significant tidal disturbances or ongoing mergers. Overall, the galaxy appears to be an evolved system with ongoing, moderate levels of star formation.
