The galaxy exhibits a clear disk structure, oriented approximately edge-on relative to our line of sight. A bulge is visible, concentrated at the center of the galaxy, appearing more smooth and uniform in color compared to the disk. There is evidence of some star formation, appearing as faint bluish regions in the disk. A redder hue is present at the far left edge. The disk appears somewhat disturbed, with some asymmetry in its outer regions, potentially indicating a past or ongoing interaction. The overall color suggests a mix of stellar populations, with a potentially older stellar population dominating the bulge and younger stars contributing to the blue components within the disk. The galaxy is relatively faint, suggesting it is somewhat distant or of lower luminosity.
