The galaxy presents as a spiral galaxy, characterized by a prominent central bulge. Two spiral arms emanate from the central bulge. They are tightly wound near the core, transitioning to a more open, medium winding as they extend outwards. There is no apparent ongoing major merger event, however it appears as if there is a minor disturbance. The color distribution indicates a higher concentration of older stellar populations towards the center, with bluer hues evident within the spiral arms, suggestive of ongoing star formation.
