The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is a significant bulge component, indicated by the bright, yellowish-white central region. The outer regions exhibit a more diffuse and fainter halo, with a slightly bluer tint, suggesting the presence of some younger stellar populations, but not in the form of defined spiral arms. There is no strong evidence of dust lanes or significant star formation regions based on this image alone. Based on its overall appearance, the galaxy appears to be in the late stages of its evolution, exhibiting characteristics of an elliptical galaxy. There is a slight possibility of a minor gravitational disturbance visible on the right side of the galaxy, but further analysis is required.
