The galaxy presents an elliptical morphology with a smooth, diffuse light profile. The core region exhibits a yellowish hue, suggesting an older stellar population likely dominated by evolved stars. Moving outwards from the core, a subtle transition to a bluer color is observed, hinting at the presence of a younger stellar population in the outer regions, or perhaps a small amount of ongoing star formation. The galaxy is not perfectly circular, appearing somewhat flattened, and is oriented at an angle to our line of sight. There is no evidence of strong spiral arm structure or significant dust lanes. The overall appearance suggests a relatively evolved system, although the subtle color gradient may indicate a more complex evolutionary history than a simple elliptical galaxy. There is no obvious sign of tidal features or recent merger activity.
