The target galaxy presents as a relatively well-defined spiral structure. Two distinct spiral arms are discernable, exhibiting a loose winding pattern as they emanate from the central region. The galaxy appears to have a moderate bulge, exhibiting an elliptical morphology in the core region with noticeable luminosity. The galaxy is not perfectly face-on, but displays a slight inclination with respect to our line of sight. There is no strong evidence of a bar feature bisecting the bulge, though a subtle elongation might suggest a weak bar structure. There is no evidence of a major merger event, although some mild irregularities in the disk structure could be indicative of minor gravitational interactions or disturbances. Overall, the galaxy displays a classic spiral morphology.
