The object appears to be a spiral galaxy, observed nearly edge-on. A prominent, bright central bulge dominates the galaxy's structure, surrounded by a fainter, extended disk. There is evidence of internal structure within the disk, but it is not possible to discern distinct spiral arm morphology from this viewing angle. The disk appears slightly warped along its major axis. The color of the galaxy is generally bluish-white, suggesting a population of younger, hotter stars. There's no obvious evidence of a strong tidal interaction or major ongoing merger. The disk appears relatively smooth, lacking prominent dust lanes or knots. The structure appears relatively undisturbed with no major signs of gravitational interaction with nearby objects. The light is brighter towards the center, becoming more diffuse towards the edges.
