The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that emits strongly in the redder wavelengths. This likely indicates an older stellar population dominating the core.

The galaxy exhibits a faint disk-like structure, which is seen through the gradient of color in the galaxy's image.

The overall color suggests a moderate redshift, and its current morphology seems relatively undisturbed, although there is potential evidence of minor disturbance due to the asymmetry in its shape.
