The galaxy appears to be a spiral galaxy, exhibiting a prominent disk structure. Spiral arms are visible, though not sharply defined; they exhibit a moderately wound morphology. The galaxy displays a small bulge in the center, not particularly prominent. There is no indication of a strong bar structure. Based on color, the galaxy is likely undergoing active star formation, with signs of HII regions. The presence of these regions indicates a relatively high rate of star formation. Some possible morphological disturbances, perhaps evidence of minor interactions or past mergers, are present. The galaxy is not perfectly symmetric, showing a slight irregularity in its overall shape.
