The galaxy presents a generally smooth and rounded morphology, suggestive of an elliptical or lenticular type. A bright, concentrated central bulge dominates the structure. The light from the galaxy appears relatively uniform, transitioning smoothly from the core outwards. The overall color profile indicates a potential mix of stellar populations. Some subtle color variations are apparent, perhaps indicating ongoing, albeit low-level, star formation activity within the galactic disk. There are no signs of major disturbances or interactions with other galaxies. 
