The galaxy presents a disk-like morphology, viewed at an angle somewhat between face-on and edge-on. A prominent central bulge exhibits a yellowish-orange hue, potentially indicative of an older stellar population. The disk component appears more complex, with hints of spiral arm structure exhibiting bluer tints, which might indicate more active star formation regions. Irregularities and faint extensions emanate from the main galactic body, hinting at possible tidal interactions or minor merger events. The overall color suggests a mixture of stellar populations, implying ongoing, albeit not exceptionally vigorous, star formation activity within a pre-existing, more evolved stellar population.
