The galaxy appears to be a single, relatively smooth structure. The morphology suggests a galaxy that is not a pure elliptical, nor a spiral with well-defined arms. The light distribution shows a somewhat symmetrical, centrally concentrated appearance. There are hints of slightly elongated structure. The color suggests the presence of an older stellar population as well as some ongoing star formation within the galaxy. There is a slightly clumpy appearance, which is expected from a galaxy with an actively forming population of stars.
