The galaxy presents as an edge-on spiral with a prominent bulge. The bulge exhibits a notably high degree of symmetry and appears to be of a rounded morphology, lacking any apparent boxiness. The disk is highly inclined to our line of sight, with minimal indication of spiral arm structure. The galaxy displays a color gradient, transitioning from a bluer hue towards the edges of the disk to a redder hue within the central bulge. This suggests older stellar populations are concentrated within the bulge, while younger, bluer stars dominate the disk. There are no visible signs of ongoing major mergers or significant tidal disturbances in this image.
