The galaxy appears to be a spiral galaxy, observed at a near face-on orientation. There is a bright central bulge, surrounded by a well-defined disk component. The spiral arms appear tightly wound around the central bulge. They exhibit a clumpy morphology suggestive of active star formation regions. The presence of a bar is suggested by the elongation and structure extending from the bulge. The outer regions of the disk fade into the background, indicating a gradual decrease in stellar density. There may be a faint ring structure or arm segment slightly detached or extended from the main disk. Overall, the galaxy demonstrates a relatively smooth and well-formed spiral structure, showing some signs of ongoing star formation.
