The galaxy presents as a relatively smooth, disk-like structure with a noticeable central bulge. It is observed at a moderate inclination, revealing a flattened shape. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. The galaxy displays a color gradient, transitioning from a yellowish-white central region to fainter, bluish outer regions. Faint spiral arm features appear to emerge from the central bulge. There is some evidence of subtle dust lanes along the disk. The overall morphology indicates a spiral galaxy, possibly of type Sa or Sb, with a well-defined bulge and moderately tightly wound spiral arms.
