The galaxy presents a predominantly smooth morphology, with a slightly elongated, elliptical shape. Its core appears luminous, suggesting a concentration of older stellar populations. The overall color is indicative of an older stellar population, implying that star formation is not currently a dominant process. There is faint evidence of a slight asymmetry and a small amount of feature disturbance, so the possibility of a minor merger cannot be ruled out. The galaxy is moderately sized, appearing neither exceptionally large nor particularly compact.
