The galaxy presents as a spiral galaxy viewed at a near-edge-on angle. There is a bright central bulge with evidence of older stellar populations, indicated by its yellowish color. The disk is visible and more bluish in hue, possibly indicating star formation, although rates are relatively low. The galaxy's structure suggests that it is relatively undisturbed, exhibiting no obvious major mergers or tidal features. There may be evidence of minor disturbances or interactions based on slight asymmetries in the disk. Overall, the galaxy appears as a relatively evolved system with a significant bulge component and ongoing, but subdued, star formation within its disk.
