The object presents as a likely spiral galaxy viewed almost perfectly edge-on. The central bulge appears prominent and somewhat elongated, potentially exhibiting a boxy shape. The dust lane is clearly visible, bisecting the galaxy along its major axis. The color suggests a relatively high redshift, with an apparent red shift in the bulge. Faint traces of spiral arms are possibly present, but obscured by the edge-on view and dust. There is evidence of minor disturbances present, and a low amount of star formation. The galaxy appears to be isolated with no obvious signs of interaction with neighboring galaxies. The galaxy's size indicates it may be of intermediate size. The color distribution suggests a higher concentration of older stars in the bulge compared to the disk.
