The galaxy presents as a relatively faint spiral system. The disk appears moderately inclined, though not quite edge-on. The central bulge is present but not particularly prominent, and the disk is the primary feature. There are prominent spiral arms visible exhibiting regions of active star formation as evidenced by the localized blue hues spread throughout the disk. There are also some dust lanes visible. The overall structure does not appear significantly disturbed, though there may be some signs of a minor interaction or past merger event based on some asymmetries in the spiral arm structure. There is evidence of a bar structure. The color indices suggest an intermediate redshift.