The galaxy presents as a relatively compact object, exhibiting a smooth, largely featureless morphology. The central region displays a concentration of light, appearing more luminous than the surrounding areas. The overall shape appears to be moderately rounded, deviating slightly from a perfect circle. There is potential evidence of a minor tidal disturbance or a small companion galaxy in close proximity, potentially interacting gravitationally with the primary galaxy. This is indicated by an apparent extension of diffuse light emanating from the main body. The galaxy emits prominently in the green to red wavelengths. It exhibits a moderate estimated stellar mass with a relatively low star formation rate.
