The galaxy presents as an elongated, disk-shaped structure with a noticeable tilt relative to our line of sight. The color gradient suggests active star formation regions, exhibiting a bluish hue. The overall structure appears relatively smooth, with no visually prominent spiral arms or significant dust lanes immediately discernible. It is possible there is some minor interaction or disturbance, although no strong evidence of merger activity is observed. The object has a relatively low mass, which is typical for galaxies of this size.
