The galaxy presents a generally smooth and somewhat rounded morphology, suggesting an elliptical or lenticular classification, but it appears to be undergoing some form of disturbance. The light profile is concentrated towards the center, with a gradual decrease in intensity towards the edges. The overall color of the galaxy is skewed towards red, which, at the measured redshift, is indicative of an older stellar population with decreased star formation. The slight asymmetry, and subtle distortions of the light distribution, implies that the galaxy is potentially interacting with another galaxy or undergoing an internal rearrangement. 
