The galaxy presents an elongated, disk-like morphology viewed nearly edge-on. A central bulge is discernible, appearing smooth and concentrated. The disk exhibits a somewhat irregular structure, lacking well-defined spiral arms. The color gradient suggests potential variations in stellar populations, with bluer hues possibly indicative of younger stars or ongoing star formation in the disk regions and redder hues in the bulge due to older stellar populations. The outer regions of the disk appear faint and diffuse, with a slight warping evident. There are no obvious signs of a major ongoing merger or strong tidal interaction, though there may be some minor disturbance in the disk structure. Overall, this galaxy appears to be a disk galaxy with a dominant disk component and a modest bulge.
