The galaxy presents as a disk galaxy, observed nearly edge-on from our vantage point. A prominent dust lane appears to bisect the galaxy, obscuring a significant portion of the central bulge. The bulge exhibits a yellowish-white hue, which indicates the presence of an older stellar population. Extending outwards from the bulge is a relatively faint disk. The disk appears to be blue, indicating ongoing star formation. There is a slight hint of asymmetry and disturbance within the disk, though overall it maintains a cohesive structure. There are no indications of a strong bar feature. The light from this galaxy suggests it is of moderate mass and has moderate star forming properties.
