The galaxy presents as a disk galaxy, observed nearly edge-on from our line of sight. The primary body appears elongated, suggesting a flattened structure consistent with a disk. A prominent central bulge dominates the galaxy's core, displaying a rounded morphology. The overall color gradient shifts from a bluer hue in the outer regions to a redder, more concentrated color within the bulge. While the disk itself lacks clear resolution, the high inclination obscures any detailed spiral arm structure. There is a distortion visible within the disk, indicating a possible gravitational interaction or recent merger event. This event is further supported by the faint tidal features that disrupt the symmetry of the disk, resulting in the irregular shape that does not conform to normal disk structures. The current activity of the galaxy is relatively low, showing little signs of active star formation. 
