The galaxy presents as an elongated, edge-on system with a distinct central bulge. The bulge exhibits a yellow to orange hue, possibly indicating an older stellar population. A faint, blueish disk is visible, extending outwards from the bulge along the major axis. This coloration could point to recent or ongoing star formation within the disk. The disk appears relatively smooth with hints of dust lanes or patchy structures along its length. No obvious spiral arm structure is discernible. There is no indication of a major ongoing merger or tidal interaction. Subtle irregularities in the disk might suggest minor disturbances, though conclusive evidence of such activity is lacking. The overall morphology suggests a disk galaxy, likely a spiral or lenticular type, viewed edge-on.
