The galaxy presents an elongated, disk-like morphology, appearing nearly edge-on from our vantage point. A central bulge is faintly visible, exhibiting a smoother, more concentrated light distribution compared to the outer regions. The disk component shows some texture suggesting the presence of spiral arms. The color gradient suggests possible ongoing star formation. The galaxy exhibits a blueish hue in the outer disk, becoming yellow-white towards the center. There is no obvious sign of major galactic mergers or tidal disruptions.
