The galaxy presents a generally elliptical morphology. There is evidence of a relatively bright central bulge or core. The light distribution appears mostly smooth across the galaxy. The galaxy exhibits a subtle, but detectable, asymmetry or possible distortion in its outer regions, particularly along what appears to be its major axis. There are indications of a potential minor disturbance. There is a suggestion of merging activity due to its morphology. The object's red-green color profile indicates that the galaxy is primarily emitting in the green and red wavelengths.
