The galaxy appears to be a spiral galaxy, exhibiting a disk-like structure. The central region shows a bright bulge, surrounded by a less luminous, fainter disk. Spiral arms are visible, though somewhat indistinct, appearing to originate from the central bulge and extend outwards. These arms seem to be loosely wound. The disk's orientation is moderately inclined to our line of sight. The color distribution suggests a mix of stellar populations, with bluer regions possibly indicating areas of active star formation within the spiral arms and a yellowish-white central bulge potentially indicative of older, more evolved stars. There are no obvious signs of strong tidal disturbances or major mergers, but the morphology suggests some minor disturbances or past interactions. The galaxy's overall structure hints at a moderate bulge and disk size.
