The galaxy exhibits a primarily smooth morphology, with a noticeable concentration of light towards the central region. This suggests a dominant spheroid component. A faint, disk-like structure may be present, though not as visually prominent as the central bulge. The galaxy's color appears relatively uniform across its structure, lacking significant color gradients or patches. The overall structure does not show clear signs of major merger events, though subtle features suggestive of minor tidal interactions cannot be ruled out based on this image alone. The galaxy likely has a mass around 10^9 solar masses. Despite its mass, the galaxy exhibits relatively low star formation activity.
