The galaxy presents a morphology that appears largely smooth and spheroid in shape. The central region exhibits a strong concentration of light, suggesting a significant stellar population density in the core. The galaxy's color appears to be generally redder, particularly within the central bulge, implying an older stellar population. There's a hint of a disk-like structure, although it's not sharply defined. Faint, diffuse light extends outwards from the core, but spiral arm structures are not readily apparent. There are no obvious signs of any major disturbances, tidal tails or ongoing mergers visible in the image.
