This galaxy exhibits a clear spiral structure, with prominent, well-defined arms emanating from a central bulge. The winding of the spiral arms appears to be relatively tight. The bulge region is bright and concentrated, suggesting a significant stellar population. There may be a weak bar structure present. The color distribution indicates active star formation within the spiral arms, but moderate to strong star formation also seems to be occurring within the bulge. There is no obvious presence of ongoing major mergers. The disk is not edge on.
