The observed galaxy presents as a spiral type, inclined at a moderate angle to our line of sight. The central bulge appears prominent, exhibiting a yellowish hue, potentially indicating an older stellar population within. Two distinct spiral arms emerge from the central region. The arms appear somewhat tightly wound, demonstrating a moderate amount of definition. The arms are not perfectly symmetrical in appearance. There is a slight degree of observed asymmetry and a notable degree of disturbance in the overall structure. There are hints of a bar-like structure traversing the central bulge. Patches of bluer light are visible within the arms. The disk itself is smooth and the galaxy does not exhibit strong features.
