The galaxy presents as an edge-on spiral. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. The disk is seen nearly edge-on, with some dust lane obscuration potentially present, though the resolution limits definitive identification. The galaxy appears to be quite massive with a rate of moderate star formation. There is a second object near the larger galaxy, possibly interacting. The bulge morphology is well-rounded. There are no strong signs of a major merger, though minor disturbances cannot be ruled out. 
