The galaxy appears as a single, diffuse light source. It exhibits a smooth morphology, lacking any clear spiral arms, bar structures, or distinct central bulge. The light distribution suggests an elliptical shape, though somewhat irregular. There is a concentration of brightness in the center that gradually fades outwards. No signs of ongoing major mergers or tidal tails are apparent, but there may be minor disturbances in the outer halo. Based on the overall appearance, the galaxy is likely a large, quiescent elliptical galaxy with a considerable stellar mass and minimal star formation activity.
