The galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent, diffuse bulge is visible at the center, exhibiting a yellowish hue, likely indicating an older stellar population. The disk itself appears thin and elongated, with hints of dust lanes obscuring portions of its light. The outer regions of the disk show a somewhat bluer tint, potentially suggesting ongoing star formation in these areas. The overall structure appears relatively undisturbed, with no clear evidence of major mergers or significant tidal distortions.
