The galaxy presents as a disk galaxy, viewed at a high inclination. The central bulge appears to be a significant component, displaying a yellowish hue, suggesting an older stellar population.  The disk is visible, although not highly resolved, and appears bluer than the central bulge. The smooth appearance, the lack of strong spiral arm definition, and the relatively bright central bulge might suggest it could be an Sa or Sb spiral galaxy. There appear to be no obvious signs of a major ongoing merger or strong tidal disturbances, and the galaxy appears relatively isolated and unperturbed.
