The galaxy presents a primarily smooth morphology, with a high likelihood of being a spheroidal galaxy. It is relatively compact and appears to be an elliptical galaxy.

The galaxy exhibits a slightly elliptical shape. There is an indication of some features that could be described as a minor disturbance, but overall it seems to be a well-defined object without major distortions indicative of an ongoing merger event.

The galaxy exhibits strong emission in the g band, suggesting active star formation. The galaxy has a estimated stellar mass of approximately 10^10.8 solar masses.
