This galaxy appears to be a relatively smooth, concentrated object. Its overall shape is somewhat elliptical, exhibiting a noticeable bulge. The color profile suggests an older stellar population, with a dominant yellowish-orange hue concentrated toward the center. There is subtle evidence of a disk-like structure, though the smoothness of the light distribution indicates it is not a strongly defined spiral galaxy. There is a slight hint of blue in the outskirts. The galaxy does not appear to be undergoing any major merging events, though there is a very slight, subtle disturbance in its morphology.
