This galaxy exhibits a clear spiral structure. Two tightly wound spiral arms emanate from a bright central bulge, which appears substantial but not overly dominant. The arms show evidence of active star formation regions, appearing slightly bluer in color than the surrounding regions of the galaxy. The overall color index of the galaxy suggests the presence of both young, hot stars and an older stellar population. The disk of the galaxy is viewed at an angle closer to face-on. There may be a weak bar structure. The general shape and appearance are consistent with that of a normal spiral galaxy undergoing typical star formation activity. There are some indications of minor irregularities in the spiral arms. The galaxy does not show any signs of major mergers or intense tidal interactions in this image.