The galaxy appears to be a spiral galaxy, viewed at a slight angle. A prominent bulge is visible at the center, surrounded by a disk. Two spiral arms are visible, tightly wound around the central bulge. The color suggests an older stellar population, with lower ongoing star formation. There are also indications of a possible bar structure within the central bulge, though the faintness and the angle may indicate a weak bar. It shows no major signs of merging.
