The galaxy presents as a relatively smooth, centralized object with a generally elliptical morphology. It exhibits a dominant yellowish-orange hue across its entirety, suggesting an older stellar population, and is compact in appearance. There seems to be no indication of strong spiral arm structures or significant dust lanes from this image alone, with a possibility of some low level merging disturbance but it is difficult to tell. This galaxy may be relatively massive with little star formation occurring in the system currently.
