The galaxy presents as a spiral type, likely a barred spiral due to a slight elongation of the central bulge. The disk exhibits prominent spiral arms, moderate in number and somewhat tightly wound, although the resolution obscures a precise determination of the arm count. The central bulge appears substantial, occupying a noticeable fraction of the galaxy's overall size. There is a clear presence of star formation occurring within the disk and the arms, as evidenced by the bluer hues scattered around. The galaxy does not exhibit signs of any major disruptive effects, such as tidal tails.
