The galaxy presents as a relatively small, inclined disk system. The color profile suggests a moderate amount of star formation, with the presence of both older stellar populations indicated by the redder core and younger, bluer stars in the arms and outer regions. There are some slight indications of possible distortions in the morphology, particularly with a warping of the disk, that could possibly be caused by a minor tidal interaction or internal dynamics. Overall the galaxy displays features of an intermediate-mass spiral galaxy.
