The galaxy presents as a spiral type, with loosely defined arm structures exhibiting a patchy, flocculent morphology. The arms demonstrate a blueish hue suggesting active star formation regions. A moderately sized central bulge is visible; it is difficult to discern its exact shape due to the image resolution but appears neither particularly dominant nor negligible in size. A bar-like structure seems to be present across the central region, possibly a strong or intermediate one. The galaxy is observed face-on, with no obvious signs of significant tidal disturbances or major mergers, although minor interactions cannot be ruled out. The outer regions of the disk gradually fade into the background sky. The object's overall form suggests a relatively late-type spiral galaxy with ongoing, but not necessarily exceptionally intense, star formation.
