The galaxy presents an elongated morphology, appearing as a flattened spheroid viewed at a significant angle relative to its rotational axis. A central bulge region is evident, exhibiting a yellow-orange hue, potentially indicative of an older stellar population. Extending outwards from the bulge, a faint, diffuse disk structure is discernible. Within the disk, a subtle bluish tint suggests the presence of younger, hotter stars. The overall structure suggests a possible late-stage merger or interaction, displaying minor disturbances in the disk's morphology. There is some evidence of tidal features or faint extended structures.