The galaxy appears to be a spiral galaxy, viewed at a slight angle relative to face-on. The central bulge is somewhat bright and ellipsoidal, but not particularly dominant in size compared to the overall galaxy. Faint spiral arms are visible, extending outwards from the central bulge into a disk, and are slightly elongated. The galaxy shows evidence of some recent or ongoing star formation, most notably in its arms. There is no significant evidence of an ongoing merger or major disturbance in the galaxy's structure, although minor disturbances cannot be ruled out. There may be a weak bar structure present across the bulge. The galaxy’s morphology appears dominated by the disk, and it does not appear to be particularly smooth.
