The galaxy presents as a spiral with a moderate-sized bulge exhibiting a yellowish hue, potentially indicating an older stellar population within. Prominent, tightly wound spiral arms extend from the central bulge, displaying distinct blue regions suggesting ongoing star formation. A slight asymmetry is observed within the spiral arms, possibly indicating a minor gravitational disturbance. The dust lanes within the arms are not clearly visible, however there appears to be a concentration of dust close to the center of the galaxy. The spiral arms are not very well defined suggesting they may be the flocculent type. There are no other visible galaxies in the field to indicate that it may be interacting with another galaxy.
