The galaxy presents as a single, concentrated object with a smooth, elliptical morphology. The central region exhibits a pronounced concentration of light, appearing bright yellow-orange, indicating an older stellar population. The outer regions show a gradual decrease in luminosity, fading into the background sky, but display little to no resolved structure in the form of spiral arms or prominent dust lanes. The shape is generally ellipsoid, appearing somewhat elongated, but not strongly so. There's a subtle hint of a disk-like structure oriented almost edge-on, as evidenced by the slight elongation and flattened appearance. No evidence of ongoing major mergers or significant tidal disturbances are apparent. The overall color suggests a relatively low rate of star formation at the present epoch.
