The galaxy appears to be a spiral galaxy, observed at an oblique angle. The disk is prominent, showing a distinct blue hue suggestive of ongoing star formation. There is an apparent central bulge that is not very pronounced. A faint bar structure can be seen across the center, but it is not particularly strong. There are hints of spiral arms, though they are not well-defined, giving the galaxy a somewhat flocculent appearance. The overall morphology indicates a galaxy undergoing some form of disturbance, potentially a minor interaction with another galaxy, as there are some irregularities in the disk structure. There is a low level of star formation activity.
