The galaxy presents a generally smooth and concentrated morphology. It exhibits a centrally dominant, bright, and somewhat diffuse core. The light profile appears to fade gradually from the center outwards, suggesting a centrally concentrated mass distribution. There's little evidence of distinct spiral arm structures or significant star formation regions within the visible portion of the galaxy. The overall shape appears close to elliptical or possibly a highly inclined disk, but the smoothness hinders detailed morphological classification from this image alone. There may be minor disturbances.
