The galaxy presents as a somewhat elongated, smooth structure, appearing generally elliptical in shape, although some asymmetry is evident. It has a diffuse appearance, with a central region that is brighter and more condensed. Faint blue hues are present in the galaxy, but the overall color is somewhat subdued. There are no strong indications of prominent spiral arms or a well-defined disk, but there is some subtle indication of substructure in the outer regions. The lack of strong color suggests the object has a lower star formation rate and the morphology is indicative of an older stellar population. There is very subtle evidence of disturbance; however, this evidence is only slight and does not present in a significant way.
