The galaxy appears to be a relatively isolated, elongated spiral galaxy exhibiting a bluish hue. The shape suggests it is viewed at a significant inclination to our line of sight. The color suggests moderate ongoing star formation. It appears somewhat disturbed, possibly indicating an interaction with another galaxy. This may be a result of either a minor or major disturbance to the galactic structure. The spiral arms may be somewhat diffuse and lack clear definition. The galaxy possesses an estimated moderate stellar mass and star formation rate.
