This galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a somewhat rounded morphology, with no immediately obvious spiral arm structures or bar features visible. The galaxy's color profile indicates a predominantly older stellar population, with a yellowish-orange hue dominating its core and extending into the surrounding halo. The overall light distribution suggests a system that is nearing the end of its star-forming activity. The galaxy seems to have low amounts of dust. There is no signs of major interactions or mergers in this image. I can observe hints of disturbance but nothing major. It is potentially undergoing only minor disturbances. The galaxy presents a fairly uniform and symmetrical structure.
