The galaxy presents as a spiral with a noticeable structure. Arms appear open and somewhat loosely wound, extending from a central bulge. The bulge exhibits a moderate size relative to the overall galactic disk. There is evidence of star formation within the arms, suggested by faint bluer hues. The disk is more prominent than edge-on in its orientation relative to our line of sight. There is a faint indication of disturbance, which suggests a potential ongoing or past interaction with another galaxy, but the disturbance does not appear to be extensive. There is also a suggestion of the presence of a bar-like structure at the core of the galaxy.
