The galaxy appears as a centrally concentrated object with a largely smooth morphology. It exhibits a generally elliptical shape, with a high degree of roundness. There are no obvious spiral arms or strong bar features visible. The overall color is somewhat redder, implying an older stellar population and suppressed star formation. No signs of a major ongoing merger are apparent, although subtle disturbances are not fully excluded at this resolution. The galaxy's relatively compact size suggests it could be an elliptical galaxy at an intermediate redshift. The galaxy's central region shows some subtle color variations, potentially indicative of residual star formation or an active galactic nucleus, though further investigation would be required to determine the precise nature of these features.
