The galaxy presents as a smooth, elliptical structure, with a dominant bulge. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. Moving outward from the core, a subtle color gradient toward greenish-blue is observed, possibly resulting from the presence of younger, hotter stars or emission line regions, though these are not distinctly resolved. There is no discernible spiral arm structure or significant dust lane obscuration. The overall morphology suggests an early-type galaxy, likely an elliptical or lenticular, with a relatively quiescent star formation history. There are no obvious signs of recent mergers or major tidal disturbances. The galaxy displays a somewhat elongated, but generally regular shape.
