This galaxy presents a relatively face-on orientation to our line of sight, exhibiting a prominent disk structure. Spiral arms are clearly discernible, although somewhat tightly wound. The central bulge is moderately sized, appearing neither overly dominant nor insignificant in relation to the disk. The overall color profile suggests a bias towards younger stellar populations, with a bluer hue apparent in the disk region, which is indicative of ongoing star formation. There is no obvious indication of major mergers or significant tidal disturbances in the overall morphology.
