The object appears to be a spiral galaxy, seen at a relatively high inclination. The disk component is prominent, exhibiting a distinct blue hue indicative of ongoing star formation. Two spiral arms are clearly visible, extending from the central region. The central bulge seems modest in size, not dominating the overall structure. Evidence suggests the presence of a bar structure across the galaxy's core. Star forming regions appear distributed throughout the disk, particularly concentrated within the spiral arms. There appears to be little to no signs of a major merger, though there are minor disturbances.
