This galaxy presents as an elongated, flattened structure, oriented approximately along its major axis. It exhibits a distinct disk-like morphology viewed nearly edge-on. A central bulge is discernible, appearing as a slightly brighter, more concentrated region. The light distribution suggests ongoing or recent star formation, as evidenced by a bluer hue throughout the galaxy, indicating the presence of hotter, younger stars. However, there is no clear evidence of spiral arm structure or prominent dust lanes. Some subtle irregularities are present in the disk's outer regions that indicate possible disturbance in the overall structure. While generally symmetrical, there are some minor asymmetries that hint at a possible minor merger or tidal interaction with another galaxy.
