The galaxy appears to be a relatively compact system with a smooth, elliptical morphology. There is a discernible central bulge. There is evidence of a fainter disk. Overall, the galaxy seems to be undergoing little active star formation, presenting mostly older stellar populations. There is a very slight disturbance in its disk, but it doesn't appear to be undergoing a major merger or interaction, with most users classifying it as undisturbed. Its round shape could indicate it is an early-type galaxy, which has slowed its rotation. Its absolute magnitudes suggest it is a galaxy smaller than our own Milky Way.
