The galaxy appears to be a single, relatively compact object. It presents a somewhat indistinct morphology, appearing largely smooth with a concentration of light in its central region. The overall shape is close to round, although there are some subtle deviations from perfect circularity. There is a suggestion of possible minor structural irregularities, which could indicate an ongoing or past interaction with another galaxy. A significant portion of the galaxy’s light output falls within the green, red, and z-band wavelengths. The galaxy exhibits relatively low star formation activity, suggesting a population of primarily older stars. The overall color suggests a well-established stellar population with some, but limited, recent star formation.
