The galaxy presents a flattened, disk-like morphology. It appears to be an edge-on or highly inclined spiral galaxy, given the elongated shape and a suggestion of a bulge in the central region. There is a distinct color gradient along the major axis, with the central region appearing brighter and with a more uniform color, transitioning to somewhat bluer regions towards the apparent edges. The overall color appears to be on the bluer end, possibly indicating the presence of younger stellar populations and ongoing star formation. There is no clear indication of well-defined spiral arms, but the clumpy appearance may suggest patchy star formation regions within the disk. The galaxy has a smooth appearance. There is a possibility of some minor interaction or disturbance, as indicated by the somewhat irregular distribution of light at the edges.
