The galaxy presents as a largely smooth, elliptical form. A central bulge is visible, appearing brighter and more concentrated than the surrounding galactic disk. The color gradient suggests an older stellar population in the core, transitioning to a bluer hue in the outer regions. The overall shape is elongated, but not dramatically so. No obvious spiral arm structures or significant dust lanes are discernible. There are some signs of minor disturbances or distortions present in the morphology of the galaxy, but it appears to be primarily settled. The galaxy appears relatively isolated.
