The galaxy presents as a fairly smooth, elliptical form, with a distinct central bulge. A subtle color gradient is visible, transitioning from a yellowish-orange core to a bluer outer halo. There are hints of what might be spiral arms, but any detailed structure is obscured by the overall smoothness and the resolution of the image. The galaxy appears to be isolated, with no obvious signs of ongoing major mergers or significant tidal disturbances. It has a substantial mass and moderate star formation rate.
