The galaxy presents as a somewhat face-on spiral with well-defined spiral arms emanating from a central bulge. The arms exhibit a patchy texture suggestive of active star formation regions. The central bulge appears relatively smooth and concentrated. There is a slight hint of a bar-like structure crossing the central region. The galaxy is slightly elongated, but overall appears quite symmetric. The disk shows a blue hue, which indicates more active star formation throughout the disk. The galaxy does not show any significant signs of merging or tidal disturbances. The overall morphology suggests an intermediate type between a spiral and a lenticular galaxy, displaying a mix of spiral arm structure and a significant central bulge.
