The galaxy presents as a relatively smooth object, with a high degree of central concentration. It exhibits a slightly elliptical morphology, appearing mostly round. The core region displays a pronounced yellowish hue, possibly indicative of an older stellar population dominating the galactic center. Moving outward from the core, the color gradient shifts towards a slightly bluer tone in the outer regions, suggesting the presence of some younger stars. The overall structure lacks distinct spiral arms or significant dust lanes, and shows no obvious signs of major disturbances or ongoing merger activity. Faint disk-like morphology.
