The galaxy appears as an elliptical-like structure, with a dominant smooth morphology. The light is concentrated towards the center, suggesting a high degree of central mass concentration. There is a slight reddish-yellow hue, possibly indicating an older stellar population with a low star formation rate. There is evidence of morphological disturbance or a potential merging event. The overall shape seems mostly rounded, with a slight suggestion of interaction. The color suggests that it is not actively forming stars.
