The galaxy presents as a spiral structure, with a dominant central bulge exhibiting a yellowish-white hue, suggesting an older stellar population. Fainter spiral arms extend outwards from the bulge, displaying a bluer color indicative of ongoing star formation. The arms appear to be wound relatively tightly around the galactic center. There is some indication of possible disturbances in the outer disk, but no obvious major merging activity is apparent. The galaxy is not seen edge-on, but rather at a more face-on angle. A subtle bar structure may be present across the central region. The overall morphology suggests moderate star formation activity within the spiral arms.
