The galaxy appears as a thin, elongated disk, presenting an edge-on orientation relative to our line of sight. The central bulge is not prominently defined, with a subtle concentration of light toward the core. The bulge morphology is somewhat rounded. The disk displays a noticeable gradient in brightness, with the central regions exhibiting a brighter, warmer hue, transitioning to a dimmer, cooler tone towards the edges. There is no strong evidence of spiral arm structure or significant dust lanes. No major disturbances or merging activity is apparent. The overall form suggests a relatively undisturbed disk galaxy.
