The observed galaxy presents as an edge-on spiral system. A prominent central bulge dominates the visual structure, appearing smooth and concentrated. The bulge exhibits a yellowish-white color, suggesting an older stellar population. A faint, thin disk extends outward from the central bulge, bisecting it horizontally. The disk appears relatively smooth, showing little evidence of distinct spiral arm structures or prominent dust lanes. The faintness and smoothness of the disk suggest that the galaxy is possibly anemic, or has reduced star formation activity. Overall, the system appears undisturbed, showing no obvious signs of tidal interactions or major mergers. The galaxy appears to be a relatively massive system.
