The galaxy appears to be a spiral galaxy, exhibiting a disk-like structure. The spiral arms are prominent, with a relatively loose winding pattern. Two main arms can be easily distinguished. There is an indication of a bar feature running through the center of the galaxy, with a moderate strength. The bulge is of moderate size, with a clear central concentration of light. The galaxy displays a blueish hue, indicative of active star formation. There are signs of possible interactions or disturbances, the galaxy appears to have undergone, or is undergoing, a minor merger or tidal interaction.
