The galaxy appears as a roughly elliptical structure with a noticeable disk-like component. There's evidence of some internal features or disturbances, potentially indicating minor interactions or internal dynamics that are impacting the morphology. The galaxy's overall color suggests a mix of stellar populations with regions that may be slightly more actively forming stars. The color distribution is somewhat uneven, possibly pointing to variations in star formation rate across the galaxy. There is a possibility that this object is undergoing some minor merging activity based on asymmetries that are visible.
