The galaxy presents a largely smooth morphology with a somewhat elliptical shape. There is no visible disk structure, spiral arms, or bar. The central region exhibits a concentration of light, appearing brighter and more intensely colored, likely indicative of an older stellar population and potentially a supermassive black hole at its center. The galaxy's color is predominantly yellow-orange, suggesting a population of older stars and potentially a lack of ongoing, significant star formation. There are subtle hints of bluer regions along the edges of the galaxy, possibly indicating pockets of younger stars, although these features are faint. No signs of major mergers or tidal disturbances are apparent. 
