The galaxy presents a largely smooth morphology, with a centrally concentrated luminosity profile. It appears elliptical in shape, although a slight elongation cannot be ruled out based on this image alone. The color gradient suggests an older stellar population, with a yellowish-white core gradually fading into a bluer halo. No prominent spiral arms or dust lanes are discernible. The overall structure indicates a system that is relatively undisturbed, with no signs of ongoing major mergers or significant tidal interactions. Star formation appears to be present but is not occurring at a high rate. 
