The observed galaxy presents as a spiral galaxy viewed almost entirely edge-on, with an estimated redshift indicating a moderate distance. A prominent dust lane bisects the galaxy's bulge, obscuring the starlight and giving it a flattened appearance. The central bulge appears bright and somewhat diffuse, with a suggestion of a rounded profile. Evident is what appears to be a companion or distorted arm structure extending from one end, showing evidence of star formation in the form of blueish hues. The disc appears relatively thin and extended. There is a very slight asymmetry. This object likely contains significant stellar mass and demonstrates ongoing star formation.
