The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It exhibits a bright, concentrated central bulge that gradually fades into an extended halo. The galaxy displays an overall yellowish-white hue, indicative of an older stellar population, with a possible region of redder, more actively star-forming region. The galaxy's morphology suggests that it has undergone significant dynamical relaxation, resulting in a largely featureless structure. There are some very slight hints of disturbances but the overall morphology is relatively undisturbed and the galaxy does not appear to be currently undergoing a major merger event.
