The galaxy presents as a spiral type, exhibiting a prominent, moderately sized central bulge. This bulge appears relatively smooth and concentrated. The surrounding disk structure displays well-defined spiral arms that appear somewhat tightly wound, suggesting a classification tending towards an Sa or Sb type spiral. These arms are characterized by regions of active star formation. There are possible signs of a weak bar feature. The galaxy does not show signs of a major merger event; however, it could be experiencing minor tidal interactions.
