The galaxy appears as a relatively smooth, elliptical-like structure. It presents a concentrated central bulge with a noticeable radial decrease in luminosity. The central region exhibits a yellowish-white hue, potentially indicating an older stellar population. A subtle blue tint is visible in the outer regions, suggesting the presence of some younger, hotter stars, although the overall color profile leans towards a more evolved galaxy. There are no discernible spiral arms or strong dust lanes visible within the galaxy's structure, further supporting the classification as a relatively smooth system. The galaxy does not display any obvious signs of a major ongoing merger or significant tidal disturbances.
