This galaxy appears to be a spiral galaxy with a prominent disk. The galaxy exhibits a central bulge of moderate size, which appears yellowish-orange in color. This indicates an older stellar population likely dominates the bulge region. Two distinct spiral arms are observed, winding moderately tightly around the galactic center. The arms show a blueish tinge, suggesting the presence of younger, hotter stars and active star formation regions. There is no obvious bar structure. The galaxy exhibits no indications of a major merger event, but there seems to be some minor disturbances.
