The galaxy presents as a spiral, viewed at a substantial inclination, close to edge-on. A prominent dust lane bisects the galaxy, obscuring a portion of the central bulge region. This bulge appears elongated and moderately bright. The disk is visible, exhibiting a clumpy structure suggesting active star formation regions. These regions appear as localized concentrations of blue light interspersed throughout the disk. The overall color gradient indicates a relatively young stellar population dominating the galaxy's light output. The presence of these distinct features indicates the likelihood of ongoing stellar evolution within this system. Further analysis could confirm the presence of more complex galactic structures.
