The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, presenting a nearly circular profile. The light distribution suggests a dominant bulge component, with a gradual decrease in luminosity outwards from the center. There's a lack of distinct spiral arms or prominent dust lanes, indicating it is likely an early-type galaxy. Faint color gradients are visible, with the central region appearing yellower, possibly indicating an older stellar population. The outer regions seem slightly bluer, suggesting the presence of younger stars, or a lower concentration of dust. There are no obvious signs of any significant mergers, tidal disturbances, or ongoing starburst activity.
