The galaxy exhibits an elongated morphology, appearing largely edge-on. It displays a prominent central bulge, which seems to be the brightest and most concentrated region. There is a disk component that extends from the bulge; though the resolution is low, dust lanes may be present, obscuring some areas of the disk. The galaxy appears relatively smooth, with no obvious signs of recent major mergers or significant tidal disturbances. The light distribution is dominated by redder colors. There is no clear evidence of ongoing star formation regions. 