The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light distribution appears largely elliptical. There is no pronounced spiral structure discernable. The galaxy exhibits a yellowish-white color gradient, with the central region appearing slightly more yellow. This suggests an older stellar population concentrated toward the core. Faint bluer regions, potentially indicative of younger stellar populations, may exist within the galaxy. A slight asymmetry could indicate minor disturbances. No significant tidal features or signs of ongoing major merger events are observed.
