The galaxy presents as a spiral type, with a moderate inclination relative to our line of sight. Two prominent spiral arms are discernible, displaying a tightly wound morphology. The central bulge appears relatively small, with a somewhat subdued color profile compared to the disk, indicating a possibly older stellar population in this region. The arms show a patchy distribution of star formation, revealed by localized blue knots. There is no apparent bar structure. The galaxy exhibits a smooth, elliptical light distribution, with an asymmetry possibly induced by interaction or uneven dust obscuration, but there are no signs of major merging features. The overall color suggests a modest rate of star formation. The shape appears moderately elongated, with its major axis several times longer than its minor axis.
