The galaxy presents a somewhat elongated morphology, significantly wider than it is tall. Its light profile is dominated by a central bulge that appears yellowish-white. This bulge exhibits a smooth texture, suggesting an older stellar population.

Extending outward from the bulge, a disk-like structure is observed, but it is seen nearly edge-on. This disk is characterized by a bluer hue. The color gradient from the bulge to the disk indicates the presence of younger, hotter stars within the disk, implying ongoing or recent star formation.

There is evidence of an interaction or merger. The presence of tidal features or asymmetries in the disk, particularly at one end of the galaxy, suggests gravitational interaction with another galaxy. The slight disturbance in the disk's shape and the presence of less prominent, extended emission further point towards a system undergoing a merging event.

Overall, the galaxy appears to be a spiral or lenticular galaxy seen edge-on, undergoing a merger or interaction, characterized by an older stellar population in the bulge and a younger, star-forming population in the disk.
