The galaxy presents as an edge-on spiral system. A prominent central bulge is visible, with a noticeable degree of roundness. The disk appears relatively smooth and displays a high inclination, obscuring any potential spiral arm structure. The disk exhibits a reddish hue, with subtle bluer regions possibly indicating areas of star formation. No major disturbances or signs of ongoing merger events are readily apparent. The galaxy's light profile suggests a significant population of older stars.
