The galaxy exhibits a clear spiral structure, with two prominent arms extending from the central bulge. These arms appear well-defined and moderately wound. Star forming regions are visible within the arms. The central bulge appears moderate in size. There's no apparent major galactic disturbance or signs of merging; though there are a few slight irregularities. The light profile suggests a mix of an older stellar population in the bulge with younger, bluer stars populating the spiral arms. The galaxy is neither fully face-on nor edge-on, but rather at an intermediate inclination relative to our line of sight.
