The galaxy appears as a moderately sized, relatively smooth, and centrally concentrated object. Its morphology suggests characteristics of an elliptical galaxy. The galaxy's shape is close to round, with a slight deviation, as it may be somewhere in between an elliptical and spheroidal structure.

There are no prominent spiral arms or a well-defined disk structure visible. It displays a smooth light distribution, lacking significant disturbances or signs of an ongoing major merger event. There might be some minor disturbance, but overall, it presents a singular, cohesive structure.

The color gradient indicates the presence of older stellar populations; however, there may be a hint of ongoing star formation, as suggested by the blueish tinge near the core. 
