The galaxy appears to be a spiral galaxy, presented at a slight angle relative to our line of sight. The galaxy exhibits a prominent central bulge, surrounded by a disk. The disk shows evidence of spiral arm structure, the arms showing an intermediate winding, with what appear to be two main arms. There may be a weak bar feature running through the bulge. The bulge appears to be of moderate size, though it appears to dominate the brightness of the galaxy. The overall color profile suggests a mixed stellar population, with a redder bulge and bluer spiral arms where ongoing star formation is likely occurring. There is no strong visual evidence of significant tidal interactions or major mergers.
