The galaxy presents as a disk galaxy observed nearly edge-on. There is some indication of a bulge component, concentrated towards the center of the disk, with a color profile slightly redder than the outer disk, suggestive of an older stellar population. The disk appears relatively smooth and undisturbed, lacking any prominent spiral arm structures or signs of a major merger event. The overall luminosity and size suggest a fairly massive galaxy. The lack of bright, blue regions indicates a low rate of star formation.
