The galaxy presents as a spiral type, although the arms are not sharply defined. The central bulge is prominent and displays a yellowish hue, suggesting an older stellar population. The disk component exhibits a bluer coloration relative to the bulge, consistent with more recent star formation. There is some indication of spiral structure present but not well-defined. The galaxy displays a fairly regular morphology, lacking any obvious signs of major merger activity, although subtle disturbances may be present. Overall, the galaxy appears to be of intermediate inclination, not viewed fully edge-on. There may be a bar structure present, however, it is not obvious from the image.