This galaxy presents as a disk-shaped structure, viewed almost perfectly edge-on from our line of sight. A prominent central bulge is visible, exhibiting a rounded morphology. The bulge appears brighter and more uniformly colored, suggesting an older stellar population. The disk component displays a subtle color gradient, shifting from a yellowish hue near the bulge to a slightly bluer tint at the outer edges. This hints at the presence of ongoing, though perhaps limited, star formation in the outer regions. The disk appears relatively smooth with no obvious signs of spiral arm structure or major dust lanes. There are subtle indications of minor disturbances in the disk, but no major merger events are evident. Overall, the galaxy appears to be a relatively undisturbed disk galaxy with a significant bulge component, characterized by a moderate mass.
