The observed galaxy presents as a spiral type, inclined at an angle such that significant disk structure is visible. The galaxy exhibits a moderate bulge component, with a relatively bright core. Spiral arms are evident, appearing somewhat flocculent and loosely wound, suggesting a possible grand-design structure. The arms appear to have some breaks or spurs. Star formation appears active within these arms, as indicated by the presence of localized color variations, though the image resolution is limiting. There is no obvious strong central bar feature visible. The galaxy appears to be relatively isolated with no signs of any recent major merger events, though there may be a faint tidal feature or minor disturbance on one side of the galaxy. Overall, the galaxy displays a typical spiral morphology with moderate star formation.
