The galaxy presents as a face-on spiral, characterized by a moderately sized bulge that diminishes into a well-defined disc. The spiral arms are prominent and appear to be tightly wound, displaying a distinct two-arm morphology. There is evidence of a bar structure extending through the central region of the galaxy. The disc exhibits a relatively smooth texture, hinting at a lack of significant star formation and minimal dust lanes. The galaxy appears relatively undisturbed, showing no significant signs of recent or ongoing merger activity. Overall, the galaxy exhibits a classical spiral structure with a moderate bulge-to-disc ratio and tightly wound spiral arms.