The observed galaxy presents as a barred spiral. It is oriented approximately edge-on relative to our line of sight. The central bulge appears prominent and somewhat diffuse, exhibiting a yellowish hue suggesting an older stellar population with minimal recent star formation activity.

The spiral arms are tightly wound and exhibit a mottled texture, indicative of both ongoing star formation regions and dust lanes. The bar structure seems to bisect the bulge and extend outwards to the inner reaches of the spiral arms. The disk appears relatively thin.
