The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a high degree of luminosity, indicating a concentrated stellar population or an active galactic nucleus. Proceeding outward, the intensity of light decreases steadily into a more diffuse halo. Subtle color variations are present, with the core displaying a warmer, yellower hue and the outer regions showing hints of bluer tones, which could indicate regions of possible recent, albeit low, star formation. There are no prominent spiral arms, bars, or other distinct features typically associated with disk galaxies. There is no strong evidence of any ongoing major merger events, although some minor disturbances or tidal features cannot be ruled out completely based on the available image resolution. The overall structure suggests that the galaxy is likely a mature system that has undergone significant dynamical relaxation.
