The galaxy presents as a flattened, elliptical shape with a bright, concentrated central bulge. The core exhibits a saturated white emission, indicating high luminosity and potentially the presence of an active galactic nucleus or a dense concentration of stars. A broader, less intense cyan-colored disk surrounds the central bulge. This disk appears relatively smooth with limited discernible structure or spiral arm features. Asymmetric and faint extension of red-shifted material is visible to the southwest. The overall morphology suggests a system undergoing gravitational disturbance.
