The galaxy presents a distinct spiral structure. Multiple spiral arms are observed, and the overall morphology suggests a barred spiral galaxy. The bar structure appears to be relatively strong, extending across a significant portion of the galaxy's central region. The galactic bulge is present, though it appears to be a moderate component of the galaxy's overall structure. A dusty disk can be identified around the bulge. There are also multiple regions of blue color within the galaxy. This may indicate more recent bursts of star formation. There appear to be very minimal signs of disturbance in this galaxy.
