The galaxy presents a generally smooth and elliptical morphology. It displays a bright, concentrated central bulge. The galaxy's light is dominated by bluer wavelengths, particularly in the core, suggesting ongoing or recent star formation. The outer regions appear less structured, gradually fading into the background. There is a slight indication of a disk-like structure, as it appears moderately flattened. No major disturbances or merging events are immediately apparent, though a minor interaction cannot be ruled out.
