The galaxy presents as a spiral type, exhibiting a moderately sized central bulge. This bulge appears yellowish, indicative of an older stellar population. The spiral arms are tightly wound around the central bulge. The arms are primarily bluish, suggesting the presence of younger, hotter stars and ongoing star formation. The disk is viewed nearly face-on. There is a slight disturbance in the spiral structure, but no major indications of a significant ongoing merger. The galaxy does not have a well defined bar.
