The galaxy appears as a spiral structure, although the arms are not sharply defined. The central bulge is prominent and exhibits a yellow-red hue, possibly indicating an older stellar population. The overall color of the galaxy shifts towards bluer shades in the outer regions, suggesting ongoing star formation. The disk is tilted relative to our line of sight, presenting an elongated shape. There are subtle signs of disturbance, such as slight asymmetries in the spiral arm structure, hinting at a possible past interaction or merger. The galaxy's light is somewhat diffuse, implying that it is not overly compact.
