The galaxy presents as an elliptical morphology, with a relatively smooth light distribution. It has an apparent reddish-orange hue, suggesting an older stellar population with fewer young, massive stars. The overall shape is slightly elongated but generally round. There are indications of some disturbances to the morphology, potentially indicative of a past or ongoing interaction or merger event, though the primary structure remains mostly coherent. There appears to be low levels of star formation in the galaxy.
