The galaxy presents as a thin, elongated disk with a prominent central bulge. The disk exhibits a slight warp, and is viewed almost perfectly edge-on, obscuring detailed spiral arm structure, if present. Dust lanes appear to be visible along the galactic plane, causing some visual dimming. The bulge has a round appearance, showing a concentration of light toward the center, likely indicative of an older stellar population. There is a gradient in color, with a subtle shift from yellow in the bulge to a bluer hue in the outer disk regions, potentially indicating ongoing or recent star formation in the disk. No major signs of tidal disturbance are visible, suggesting no recent major merger events. However, there is some unevenness in the disk light distribution that is indicative of a minor disturbance. The galaxy overall appears to be relatively isolated.
