This galaxy appears to be a somewhat diffuse object, exhibiting a mixture of features suggestive of an intermediate stage of morphological classification. The light distribution is not entirely smooth; however, neither does it display prominent spiral arms or a well-defined disk structure. There is a central concentration of light that graduates into a less concentrated halo. There is a hint of disturbance in the morphology, possibly due to a minor interaction or recent merger. Colors indicate a possible mixture of stellar populations, with some regions exhibiting bluer hues which would suggest younger, hotter stars, and other regions exhibiting a more redshifted, orange hue suggestive of older, cooler stars.
