The galaxy appears as a relatively smooth, rounded object. It exhibits a concentration of light towards its center, suggesting the presence of a bulge. While the image resolution is limited, there is no obvious presence of spiral arms or a well-defined disk structure. The galaxy's color appears somewhat redder, possibly indicating an older stellar population, reduced star formation activity and higher mass. There appears to be no significant signs of ongoing mergers or major disturbances in its overall structure. The light is distributed quite uniformly.
