The observed galaxy presents as a spiral, although its orientation appears somewhat edge-on, limiting clear observation of its full morphology. The central bulge exhibits a moderate size, displaying a concentrated region of older stellar populations, as indicated by its yellowish hue. Fainter, bluer regions are seen scattered throughout the galaxy, potentially indicating ongoing star formation. Two primary spiral arms are discernible, though obscured in the center. It shows a normal winding pattern. Overall, the galaxy shows no obvious signs of major interaction or disturbance.
