The galaxy presents as a relatively faint, elongated structure, suggestive of a disk galaxy viewed edge-on. A noticeable dust lane bisects the galaxy along its major axis, obscuring light from the galactic bulge and contributing to its relatively faint overall appearance. The bulge appears modest in size. The disk exhibits a smooth profile, with the outer regions fading gradually into the background. The blue hue, particularly noticeable in the disk region, indicates the presence of recent star formation. Some clumpy regions are present, representing areas of active star formation or obscured regions within the disk. The overall morphology suggests a galaxy that has not undergone any recent major mergers. The galaxy appears undisturbed.
