The galaxy presents a generally smooth appearance, suggesting an elliptical morphology. The light distribution exhibits a centrally concentrated bulge. There is some evidence of a disk-like structure, though it is faint, and the bulge is dominant. Its overall shape is moderately elliptical, appearing somewhere between round and elongated. There may be evidence of a minor disturbance, but there are no clear signs of on-going major merging activity. Based on its color, the galaxy has moderate mass and a relatively low star formation rate.
