The galaxy presents an elliptical morphology, though with some suggestion of a disk component. The light distribution appears relatively smooth with a bright central bulge and no prominent spiral arms. The color gradient suggests older stellar populations dominating the bulge with possible ongoing star formation in the outer regions of the disk, indicated by slightly bluer colors. There is a possible interaction or minor disturbance visible, seen as a slight asymmetry in the outer regions of the galaxy. The overall structure appears largely unperturbed, suggesting that if a merger is occurring, it is in its early stages, or is a minor interaction.
