The galaxy appears as a centrally concentrated object, exhibiting a morphology that leans towards smooth. It has a generally round shape, although there might be slight deviations from perfect circularity. There's a noticeable, brighter core or bulge region, indicating a higher density of stars in the central area. The overall color seems to have some variance, possibly indicating different stellar populations within the galaxy. The outer regions of the galaxy appear fainter and more diffuse, suggesting a gradual decrease in stellar density with increasing distance from the center. There is a hint of some mild disturbances in the galaxy's structure, perhaps due to tidal interactions or past mergers, but this is not a strongly dominant characteristic.
