This galaxy appears to be a spiral galaxy viewed edge-on from our perspective. The disk is visible as a thin, elongated structure, displaying a reddish-orange hue throughout. A central bulge is visible, appearing somewhat bright and concentrated. The bulge seems to be more rounded in shape. A potential minor disturbance is seen in the disk, possibly a small irregularity. The overall morphology suggests a relatively undisturbed system, not currently undergoing a major merger event. The color of the disk suggests a population of older stars, with ongoing star formation.
