The galaxy presents as a highly inclined, edge-on spiral. A prominent central bulge is visible, although its exact morphology cannot be determined due to the edge-on perspective. Dust lanes appear to bisect the galaxy along its major axis. Star formation appears prevalent, especially along the edges, contributing to the blue hue observed. Based on the limited visual data, there's no immediate indication of any major merger events or tidal disturbances. The galaxy displays a generally smooth, elongated profile.
