This galaxy presents a clear edge-on disk morphology. The central bulge is prominent and appears somewhat elongated, possibly resembling a rounded or elliptical structure. There are hints of dust lanes visible, particularly along the galactic plane. The disk shows a subtle color gradient, with bluer hues visible at its outer edges. This suggests ongoing star formation in the outer regions, while the central bulge exhibits a yellower-redder color, indicative of an older stellar population. The overall structure appears relatively undisturbed, without any obvious signs of major merging events or significant tidal distortions. Some minor irregularities are visible, which may be associated with minor disturbances.
