The galaxy presents as an elliptical morphology with a smooth appearance. The primary body is a bright, concentrated spheroid, exhibiting a yellow-orange hue that suggests an older stellar population, and appears to be fairly quiescent. A subtle halo of light extends outwards from the main body, diminishing in intensity and suggesting a more diffuse distribution of stars. There are hints of a possible slight asymmetry or a very faint tidal feature extending from one side, although the image resolution makes definitive confirmation challenging. There are no readily apparent dust lanes, spiral arms or knots of star formation visible. The galaxy appears relatively isolated and undisturbed.
