The object appears to be a spiral galaxy viewed at a near edge-on orientation. A central bulge is visible, appearing relatively smooth and concentrated. The disk of the galaxy exhibits a blue hue, suggestive of ongoing star formation. There is some evidence of dust lanes or irregular structures within the disk, though the resolution limits a detailed analysis. The overall shape is elongated, consistent with a flattened disk structure. No significant tidal features or signs of a major merger are readily apparent. There may be some minor disturbances in the disk, but they appear subtle.
