The object appears to be a spiral galaxy, viewed almost perfectly edge-on. There is a prominent central bulge that is significantly brighter and exhibits a yellow-red color, suggesting an older stellar population. The disk is thin and elongated, with a subtle blue tint, indicative of younger, hotter stars and ongoing star formation. The disk appears relatively smooth with only a few small irregularities. The overall structure suggests a well-defined and relatively undisturbed morphology. The galaxy shows no obvious signs of a major ongoing merger or strong tidal interactions.
