The galaxy presents a predominantly smooth morphology, suggesting it is likely an elliptical or lenticular galaxy. The shape appears to be somewhere in between round and elliptical, leaning closer to an elliptical shape. The color gradient indicates a relatively older stellar population, as evidenced by the reddish-yellow hue concentrated in the central bulge, and the subtle blue around the edges. This indicates that the galaxy is likely not undergoing rapid star formation at this time. There appears to be a small amount of visible disturbance and potential merging activity.
