The galaxy appears to be a spiral galaxy, viewed nearly edge-on. A central bulge is visible, exhibiting a yellowish-orange color indicative of an older stellar population. The disk surrounding the bulge shows a bluer hue, suggesting the presence of younger, hotter stars and potentially ongoing star formation. The galaxy presents with a level of asymmetry or disturbance in its morphology, hinting at possible past interactions. There is no obvious sign of major mergers. The galaxy's disk appears relatively smooth and tightly wound, though some minor irregularities may exist.
