The galaxy presents as a spiral type, seen at a slight angle relative to edge-on. The presence of spiral arms is apparent, though not sharply defined. The arms exhibit a moderately wound structure. A central bulge is present, though not overwhelmingly dominant, appearing of moderate size relative to the galactic disk. No strong bar structure is visible, with only a possible faint bar. There does not seem to be any major merging taking place, however, there is a possible minor disturbance. The galaxy appears to be relatively massive and actively forming stars.
