The galaxy presents as a spiral galaxy, viewed at an oblique angle. The nucleus appears bright and yellowish, suggesting a population of older stars. Spiral arms are discernible, exhibiting a moderate winding. The disk shows a mottled texture, likely due to dust lanes and star-forming regions. There is an apparent asymmetry within the disk, potentially indicative of a minor disturbance or interaction with a smaller companion. The color gradient across the galaxy suggests ongoing star formation within the spiral arms. The overall morphology suggests an intermediate-sized spiral galaxy.
