This galaxy presents as an edge-on spiral, characterized by a prominent central bulge. The bulge exhibits a yellowish-orange hue, indicative of an older stellar population. Extending outwards from the bulge is a disk, appearing relatively thin and elongated due to the edge-on orientation. The disk appears less defined with respect to the bulge and is tilted on the x-axis. A region of active star formation can be seen as a knot of increased brightness in the lower portion of the disk, perhaps indicating a more active region of gas ionization or concentration of young, hot stars. The overall morphology suggests that the galaxy is relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions.
