The galaxy presents as a disk galaxy, oriented nearly edge-on from our perspective. There is a central bulge that appears somewhat elongated and concentrated, exhibiting a yellowish hue. The disk component is visible as a flattened structure extending outwards from the bulge, with a noticeable blue tint, indicating potential star formation activity. The disk appears to be relatively smooth, showing little evidence of strong spiral arm structure or major disturbances. The color gradient suggests a possible difference in stellar populations between the central bulge and the outer disk regions. From this limited data, the presence of a boxy bulge and merging features is not definitively supported. Overall, the galaxy appears to be a relatively quiescent, edge-on disk galaxy.
