The galaxy exhibits a flattened, elongated morphology, likely an edge-on or highly inclined disk galaxy. A bright, concentrated central bulge region is observed, with light possibly indicating an active galactic nucleus. The disk component shows faint hints of spiral arm structure, albeit diffuse and not well-defined. The dust lanes are not distinctly apparent, but some localized color variations suggest obscuration. Overall, the galaxy presents a relatively smooth appearance, with no obvious signs of major recent merger activity. The overall color is leaning towards the red side, indicating an older stellar population and low levels of recent star formation.
