The galaxy presents an elongated, somewhat spindle-like morphology, suggesting it could be an edge-on spiral or a lenticular galaxy. The central bulge appears prominent and exhibits a yellowish-orange hue, which may indicate an older stellar population. Moving outward from the core, a bluer color is visible. The disk appears relatively smooth with some clumpy features, possibly regions of recent or ongoing star formation. No strong evidence of spiral arms is visible in the image, this could be due to the edge-on orientation. There also seems to be a hint of a dust lane, which could be obscuring some of the underlying galactic structure.