The galaxy presents as a relatively smooth, centrally concentrated object. It appears largely elliptical in shape, with a slight deviation towards a more rounded form. The central region displays a bright, yellowish-white core, suggestive of an older stellar population and potential presence of a supermassive black hole. Moving outward from the core, the galaxy gradually transitions to a bluer hue in the outer regions, potentially indicative of more recent or ongoing star formation in those areas, though at a low rate. There is no clear evidence of spiral arms or a distinct disk structure, nor any indications of a major merger event or significant tidal disturbances. Overall, the galaxy exhibits a morphology consistent with an early-type galaxy undergoing modest star formation.
