The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, trending towards a more rounded appearance, with a distinct core region that displays a warmer, redder hue, likely indicating an older stellar population. This central region is surrounded by a more diffuse halo exhibiting a cooler, greenish-yellow color, potentially indicating younger stars or ongoing star formation at a relatively low rate. There are no obvious signs of spiral arms or a disk structure. There is no clear indication of any major merger events or significant disturbances in its morphology, although there may be very minor asymmetry or irregularities in the outer regions.
