The galaxy presents as an edge-on spiral or lenticular system. A prominent central bulge is observed, exhibiting a smooth, concentrated luminosity profile. The disk appears thin and elongated, with a relatively uniform surface brightness. The overall color gradient transitions from a yellowish/orange hue in the bulge to a slightly bluer shade in the outer disk, suggesting potential variations in stellar populations and ongoing star formation activity within the disk. There is no immediately apparent evidence of strong dust lanes, tidal features, or significant morphological disturbances indicative of recent major mergers, however there appears to be some minor disturbance. The bulge has a rounded morphology, with a high likelihood of not being boxy.
