The observed galaxy presents as a significantly elongated structure, viewed nearly edge-on. Its morphology suggests a spiral or lenticular galaxy. A prominent dust lane, visible as a dark reddish band, runs along the major axis, obscuring some of the central galactic bulge. The bulge appears relatively small and centrally concentrated within the disk. The disk component shows a smooth light distribution, becoming fainter towards the edges. The galaxy has relatively high HI content with good signal to noise, suggesting possible star forming activity. The overall color suggests the presence of both younger stellar populations associated with star formation regions and an older, redder population distributed throughout the disk and bulge. The galaxy shows a possible minor disturbance, possibly associated with an ongoing minor merger. 
