The galaxy exhibits a clear disk morphology, viewed at an oblique angle to our line of sight. Tightly wound spiral arms are observed throughout the disk, however their arm count is indiscernible due to the angle. There is a very faint, possibly weak bar visible in the center of the galaxy. A moderately sized bulge is present, exhibiting a yellowish hue, suggesting an older stellar population compared to the disk. The galaxy appears relatively isolated with no major signs of tidal disruption, or interaction with other galaxies. The spiral structure indicates ongoing star formation within the disk, which is supported by bluer colors within the disk. The dust lanes, although not prominent, appear to be present, contributing to the somewhat mottled appearance of the disk. The outer regions of the galaxy appear fainter and less defined, likely due to decreasing stellar density. The relatively smooth and continuous light distribution suggests the galaxy is not undergoing a major merger, though minor disturbances cannot be ruled out.
