The galaxy appears as a moderately bright, disk-shaped structure, viewed nearly edge-on. The central region exhibits a concentrated bulge of brighter, whiter light, suggesting a relatively dense stellar population. A distinct dust lane bisects the galaxy horizontally, obscuring light from behind and indicating the presence of interstellar medium. This lane shows up as a blueish-green band of color. The presence of reddish hues towards one edge of the galaxy may indicate a region of active star formation. Overall, the galaxy's smooth profile suggests a lack of recent major mergers or significant tidal interactions. 
