The galaxy appears to be a spiral galaxy, viewed at a significant inclination, appearing nearly edge-on. There is a prominent, relatively bright central bulge. The disk shows evidence of dust lanes and some clumpy structures, suggesting active star formation. The color gradient indicates that the bulge is redder than the disk. The disk exhibits some distortions, possibly indicating a minor gravitational interaction, or perhaps internal instabilities. The galaxy's features suggest it is a relatively massive system with moderate star formation activity.
