The galaxy presents as an elliptical morphology, exhibiting a smooth light profile with a high degree of central concentration. Its core appears bright and yellowish, suggesting an older stellar population and relatively low levels of on-going star formation. The isophotes appear generally regular, although with some minor disturbances. The galaxy's overall structure seems to be undisturbed, indicating that it is not undergoing a major merger event. There is no evidence of spiral arms or a prominent disk. The galaxy has a low star formation rate. The overall color suggests that it may be an early-type galaxy.
