The galaxy presents a spiral morphology, characterized by a central bulge and spiral arms extending outward. The arms appear tightly wound, indicating a potentially higher angular momentum. The bulge appears relatively small, but it is still very bright. Faint signs of star formation are hinted at, based on the galaxy's colors and the presence of the spiral arms. Evidence for the presence of a bar is unclear from the image. There is no indication of a major merger or significant interaction with other galaxies. The estimated size suggests a moderate to large spiral galaxy.
