This galaxy exhibits a distinct spiral structure, oriented approximately face-on relative to our line of sight. The spiral arms are well-defined and extend outwards from a central bulge. The winding of the spiral arms appears relatively tight, and there seem to be approximately 3-4 arms. The central bulge is a moderate size, and appears somewhat luminous. There appears to be no strong bar structure. The colour profile suggests that it may have a relatively high star-formation rate. The galaxy does not appear to be strongly interacting with other galaxies, though there are some disturbances visible in the spiral arm structure that may hint at a minor disturbance due to a past interaction or merger. The overall morphology suggests that this galaxy is a fairly typical spiral galaxy.
