The galaxy presents as a spiral galaxy exhibiting a prominent disk structure. Spiral arms are apparent, and the morphology suggests a grand design with tightly wound arms.

A central bulge is noticeable but appears to be relatively moderate in size. The galaxy exhibits a bar structure. Dust lanes may be present within the spiral arms, obscuring some of the underlying stellar population. The overall color profile indicates the presence of both older stellar populations within the bulge and younger, bluer stars in the spiral arms, suggesting ongoing star formation. The galaxy does not appear to be undergoing any major mergers, however, there are minor disturbances.
