This galaxy appears to be a spiral galaxy, exhibiting a prominent disk structure. The disk displays a notable inclination relative to our line of sight, allowing for a partial view of its spiral arm morphology. Faint spiral arms extend outwards from a central bulge. The central bulge appears moderate in size. There appears to be evidence of a stellar bar structure spanning a substantial fraction of the galactic core region. The galaxy exhibits a general bluish tinge in the spiral arms indicating populations of younger, bluer stars. The overall morphology of the galaxy appears relatively undisturbed, lacking evidence of recent major mergers. The winding of the spiral arms appears intermediate, not tightly wound nor loosely structured. There appears to be around two major arms.
