The galaxy presents as a spiral type, exhibiting distinct spiral arm structures. The arms are tightly wound around a central bulge, with some asymmetry and a moderate bulge size. The spiral arms display a bluer hue, indicative of ongoing star formation, while the bulge appears more yellowish, suggesting an older stellar population. There are no major signs of an ongoing or recent merger event, although some minor disturbances may be present in the outer disk. The galaxy is oriented somewhat face-on, allowing a relatively clear view of its spiral structure. The system exhibits a degree of barred structure in the central region. Overall, the galaxy appears to be a relatively well-defined spiral galaxy with evidence of active star formation within its arms.