The galaxy presents as a flattened, elongated structure, suggesting a disk morphology viewed nearly edge-on. A central bulge component is discernible, exhibiting a somewhat rounded shape. The disk shows a distinct color gradient, with bluer hues along the outer edges indicative of regions with more active star formation. The central regions appear yellower and redder, potentially representing a population of older stars. The galaxy does not appear to be significantly disturbed, but the disk shows some asymmetry, possible hinting at past interaction or internal processes. There is no clear evidence of a major ongoing merger. The galaxy's overall shape and color distribution are broadly consistent with that of a spiral galaxy seen edge-on.
