The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, symmetrical morphology. Its overall color is yellowish-white, suggesting a stellar population dominated by older, redder stars. There is a slight elongation to the galaxy's shape, indicating it is not perfectly spherical. No distinct spiral arms or prominent dust lanes are discernible. The galaxy's light is centrally concentrated, with a gradual decrease in brightness towards the outer edges. No signs of active galactic nuclei or intense star formation regions can be definitively identified based on this image. There is no obvious presence of any tidal tails or significant distortions indicative of a recent major merger event, although minor disturbances cannot be ruled out at this resolution. The smooth and symmetrical appearance points towards a relatively relaxed, evolved system.
