The galaxy presents as a relatively smooth, disk-shaped system, oriented roughly edge-on to our line of sight. A central bulge is visible, exhibiting a yellowish hue suggestive of an older stellar population. The disk component shows a bluer tint, potentially indicating ongoing star formation. There is some evidence of faint, extended structure within the disk but no obvious spiral arm features are discernible in the image. Based on the observed morphology, it is most likely a spiral galaxy, potentially of type Sa or Sb. No major interactions or merger activity is obviously perturbing the structure.
