This galaxy presents as a disk galaxy, observed nearly edge-on from our line of sight. The central bulge appears prominent and elongated, with a primarily rounded morphology. There is a clear disk structure, with relatively little dust obscuring the main body of the galaxy. The disk exhibits a smooth appearance overall. The color profile shows a concentration of older, redder stars within the bulge. The disk contains regions of blue light, indicating areas of active star formation. No significant tidal features or other signs of major mergers are observed. There may be evidence of minor disturbances.
