The galaxy presents as a spiral type, with a notable disk structure. Spiral arms are clearly visible, exhibiting a tightly wound morphology. These arms display a predominantly bluish hue, suggestive of ongoing star formation. The galaxy possesses a moderately sized central bulge, which appears yellowish, indicating an older stellar population. There is no evidence of a strong bar structure. A slight asymmetry or minor disturbance is observed in the spiral arm structure.
