This galaxy appears to be a spiral galaxy, viewed at an oblique angle, but not quite edge-on. There is evidence of spiral arm structure, though the arms are somewhat flocculent and not tightly wound. The central bulge appears moderately sized, exhibiting a yellowish color, suggesting an older stellar population. A bar structure is suspected, although it is not very pronounced. The disk component shows a bluer hue, consistent with younger stars and ongoing star formation, albeit at a low rate. The overall morphology suggests a relatively undisturbed system, with no obvious signs of major recent mergers. Minor disturbances cannot be ruled out.
