The galaxy presents as a slightly elongated, centralized structure with a high degree of smoothness, suggesting a potential classification as an elliptical galaxy, or possibly a lenticular galaxy seen at an angle. The central bulge is bright and dominates the light profile, with a yellow-orange color, implying an older stellar population.

There is a hint of a fainter, bluer extension on one side, possibly indicating recent star formation or interaction with another galaxy. The overall morphology suggests it is more elliptical than disk-dominated. There is a hint of what might be a minor disturbance in the form of asymmetry, though it's not pronounced enough to suggest a major ongoing merger.
