The galaxy presents a prominent spiral structure. Distinct, albeit somewhat tightly wound, spiral arms are observed extending outwards from the central region. The color gradient across the arms suggests active star formation. The central bulge appears moderate in size relative to the overall galactic disk. A bar-like structure seems to be present but is not strongly defined. The disk is oriented at a slight angle relative to our line of sight. There is no obvious evidence of a major ongoing merger, however there is a possibility that a smaller merger or tidal interaction may be taking place.