The galaxy appears to be a spiral galaxy, although its spiral arms are not sharply defined, exhibiting a somewhat flocculent structure. There is a central bulge that seems relatively prominent and somewhat spheroidal in shape, with a yellowish-white color, indicating an older stellar population. The disk of the galaxy appears tilted relative to our line of sight. The bluer regions within the disk suggest areas of recent star formation. Overall, the galaxy presents a rather smooth appearance with a few faint indications of disturbances to its shape, possibly due to minor gravitational interactions.
