The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. The galaxy appears to be generally rounded in shape, with only a slight elongation. There are no readily apparent signs of spiral arm structures or significant dust lanes. Color gradients suggest a relatively uniform stellar population, with a possible presence of older stars. Overall the galaxy seems undisturbed, displaying no major signs of any current or recent major merger events.
