This galaxy exhibits a generally smooth morphology, appearing somewhat elliptical in shape. The central region is substantially brighter and more compact, suggesting a concentrated nucleus. Moving outward from the center, the luminosity decreases gradually. Subtle color variations are present throughout the galaxy. There is a slight indication of asymmetry in the galaxy's structure. It is possible this galaxy may have had a prior merging event. The outer edges of the galaxy appear somewhat irregular, indicating potential tidal disturbances. Despite the relatively smooth overall appearance, there are hints of underlying features or structures that might be revealed with higher resolution imaging.