The galaxy appears to be a spiral type, presenting with a disk-like structure, and likely exhibiting spiral arms. There is an indication of a bar feature spanning the central region. The galaxy's bulge is moderately sized relative to the disk. Some regions of active star formation can be observed across the arms. The disk appears more inclined and is not a face on galaxy. Based on its morphology, there does not appear to be any ongoing major merging events, but there may be a minor disturbance present. The galaxy exhibits redder colors in the central bulge region, suggesting an older stellar population, while bluer colors are present in the disk and spiral arms, consistent with younger stars and ongoing star formation.
