The galaxy presents as an edge-on spiral, with a significant bulge component. The bulge appears smooth and somewhat rounded. The disk is visibly elongated and thin, with a high degree of inclination relative to our line of sight. Some evidence of internal structure can be seen within the disk, but no distinct spiral arms are discernible. The galaxy exhibits a yellowish-orange hue in the central bulge, suggesting an older stellar population. The disk appears to have a bluer component, possibly indicating ongoing star formation. There are no signs of major mergers or tidal disturbances. The galaxy's morphology suggests that it has a relatively large stellar mass and a moderate rate of star formation. Overall, the galaxy appears to be a well-defined, relatively undisturbed system.
