The galaxy presents as a highly inclined, edge-on spiral galaxy. The central bulge appears relatively bright and concentrated, displaying a yellowish-white hue, possibly indicative of an older stellar population. Fainter, bluish regions extend outwards from the central bulge. The spiral disk is elongated and appears thin, exhibiting a clear dust lane that bisects the galaxy along its major axis. These regions suggest ongoing star formation, particularly near the edges of the disk. The galaxy's overall morphology indicates a well-defined structure with a high degree of rotational symmetry. There are no obvious signs of major mergers or significant tidal disturbances.
