The galaxy exhibits a distinct disk-like morphology, with prominent spiral arm structures. The arms appear relatively tightly wound, and a moderate-sized bulge is clearly visible at the galaxy's center. There are possible disturbances in the disk indicating a non-negligible fraction of merging activity. The galaxy's overall color suggests an intermediate age stellar population, with indications of ongoing star formation in the spiral arms. There is no strong bar feature observed within the galaxy. The disk is not edge on, but at a considerable angle. The galaxy has an elliptical appearance with the major axis oriented at approximately 160 degrees. 
