The galaxy presents as a spiral type, with a defined central bulge from which spiral arms emanate. The spiral arms appear tightly wound. Star formation is actively occurring, with regions of intense blue emission observable within the spiral arms, indicative of hot, young stars. The galaxy shows no signs of a major merger or significant tidal disturbances. The overall structure appears relatively symmetric, suggesting it is in a fairly settled state. A small bar feature may be present in the center.
