The galaxy exhibits a spiral morphology, with tightly wound spiral arms that are clearly visible but somewhat diffuse. The central bulge appears prominent and is characterized by a yellowish hue, suggesting an older stellar population. The galactic disk presents a bluish tint, likely indicating the presence of younger, hotter stars and ongoing star formation. The galaxy appears to be inclined relative to our line of sight, not quite edge-on but far from face-on. There is subtle evidence of asymmetry in the spiral arm structure, potentially hinting at past interactions or internal dynamic processes. The overall shape of the galaxy is elliptical, with a semi-major axis longer than its semi-minor axis.&#x20;
