The galaxy presents as a spiral type, oriented approximately face-on relative to our line of sight. It exhibits a notable disk structure with prominent spiral arms. Two main spiral arms appear to dominate, exhibiting a medium winding pattern. The arms display a clumpy morphology, suggesting regions of active star formation. A central bulge is visible, appearing moderate in size. The bulge exhibits a yellowish hue, implying a population of older stars. The disk shows a bluer color indicative of younger stars. There is no strong evidence of a bar structure in this galaxy. There is some evidence of minor disturbance, which may indicate a potential ongoing or past merger event. Overall, the galaxy appears to be an actively star-forming spiral galaxy with moderate signs of interaction.
