The galaxy presents as a relatively bright spiral system, viewed at a shallow angle. Its nucleus is well-defined and appears yellowish, indicating a population of older stars. The galaxy has a well-defined disk structure with hints of spiral arms. The spiral arms are tightly wound and there is a moderate amount of light from the blue stars in the spiral arms. It does not show any sign of disturbance by any merging or galaxy interaction. The bulge constitutes a moderate size.
