The galaxy presents as a spiral galaxy, observed at an oblique angle. The structure is dominated by a prominent central bulge, surrounded by a well-defined disk. Within the disk, two distinct spiral arms are visible, exhibiting a medium winding. The arms appear somewhat flocculent. The central bulge exhibits a moderate luminosity, appearing slightly brighter than the disk. The spiral arms display a mottled texture, suggesting areas of active star formation. The overall color is consistent with a mix of stellar populations, with some bluer regions indicating younger stars, and redder regions indicating older stars or dust obscuration. There is a slight suggestion of a bar feature crossing the central bulge, though it is not overwhelmingly prominent. The galaxy appears relatively isolated, with no clear signs of major interactions or mergers, though there are some asymmetries which indicate minor disturbances.
