The galaxy presents as an elongated, edge-on spiral system. A central bulge is visible, appearing relatively smooth and concentrated. The disk component extends significantly outward from the bulge, exhibiting a flattened morphology consistent with a high inclination angle relative to our line of sight. The disk displays evidence of substructure, hinting at spiral arm features although these are not clearly resolved, likely due to the edge-on orientation. The galaxy exhibits a bluer hue in the outer regions of its disk, suggestive of ongoing star formation activity. Overall, the galaxy appears to be relatively undisturbed, showing no obvious signs of recent major merger events. Based on the HI properties, the galaxy possesses a notable amount of neutral hydrogen.
