The galaxy presents as a spiral type, viewed at a shallow inclination relative to our line of sight. Spiral arms are visible, though somewhat diffuse and not sharply defined. The overall color suggests a mix of stellar populations. A central bulge is present, exhibiting a slightly yellowish hue, potentially indicating a higher concentration of older, cooler stars. The spiral arms appear bluer, hinting at ongoing star formation. The galaxy does not show any significant signs of major merger activity.
