The galaxy appears as a relatively faint, elongated object. It is likely a spiral galaxy seen nearly edge-on, as the disk structure is noticeably flattened. There's evidence of a central bulge with a somewhat yellowish or reddish hue, suggesting an older stellar population concentrated towards the core. The outer regions of the disk appear more diffuse and slightly bluer, indicating the presence of younger stars and possible ongoing star formation. No prominent spiral arms or dust lanes are clearly visible, likely due to the high inclination angle. The galaxy seems relatively undisturbed with no signs of major mergers.
