The galaxy presents a predominantly smooth morphology, appearing largely featureless. Its shape is notably round, showing no significant elongation or asymmetry. The color profile suggests a central concentration of older stellar populations, indicated by the yellowish hue in the core region. The outer regions display a gradual color transition to a bluer tint, possibly indicating the presence of younger stars or ongoing star formation, albeit at a low rate. No signs of tidal disturbances, major mergers, or significant structural irregularities are discernible. The overall impression is that of a relaxed, relatively undisturbed galaxy, possibly an elliptical or lenticular type.
