This galaxy exhibits a predominantly smooth morphology, with a high degree of central concentration. The color profile indicates an elliptical classification, with the core appearing markedly more yellow, potentially indicative of an older stellar population and reduced star formation activity. The outer regions display a more diffuse, slightly bluer hue, suggesting a younger stellar population within the galaxy's extended halo, though star formation is still low. The overall shape is largely round, lacking any significant asymmetries or signs of recent major merger events. Minor irregularities might be present, possibly the result of small disturbances within the galactic structure.
