The galaxy presents as a diffuse, somewhat amorphous structure, exhibiting a primarily blue hue. The central region appears slightly more condensed but lacks a clearly defined, bright nucleus, suggesting a small or non-existent bulge. Spiral arms are visible, exhibiting a somewhat disorganized, flocculent morphology rather than grand, sweeping designs. A faint bar structure may be present, though it is not prominently defined. There is evidence of active star formation occurring in the disk. Some level of disturbance or merging activity with smaller companions cannot be ruled out. The galaxy is observed nearly face-on and is relatively compact in apparent size.
