The galaxy presents as a spiral, viewed at a significant angle approaching edge-on. Two prominent, loosely wound spiral arms extend from a central bulge. These arms appear somewhat asymmetrical in their structure. The bulge exhibits a yellowish hue, possibly indicating an older stellar population. The spiral arms show areas of bluer light, suggestive of more recent star formation. There appear to be no major disturbances in the galactic morphology, although the asymmetrical arm structure could indicate a minor gravitational interaction in the past. A bar structure is not strongly apparent in the image, but it is difficult to determine without a clearer view. The galaxy's disk is evident and forms a distinct plane of light, indicating a flattened structure as expected for spiral galaxies.
