The galaxy presents a complex structure, appearing to be a spiral type. It possesses a moderate-sized bulge, which displays a yellowish hue, indicative of an older stellar population. Extending from the central bulge are well-defined spiral arms. These arms appear to have a medium to loose winding pattern, suggesting they are not tightly wound around the galactic center. The spiral arms exhibit a bluer color, implying the presence of ongoing star formation regions. The galaxy appears to have undergone, or is currently undergoing, a minor interaction or disturbance with a smaller companion galaxy. There is no obvious dust lane present.
