The galaxy presents as a spiral type, viewed at an oblique angle, exhibiting a generally disk-like structure. Evidence of spiral arms is apparent, though the inclination complicates precise quantification. These arms show a moderate degree of winding tightness. The central bulge is moderately sized. Patches of enhanced blue luminosity are distributed throughout the disk, likely indicative of ongoing star formation regions. There is evidence of a possible bar feature crossing the bulge. There are possible tidal disturbances from either a merger or past interaction with a different object. There are blue knots on both sides of the galaxy.
