The galaxy presents as a flattened, disk-shaped structure observed edge-on. The dominant color is a pale blue, suggesting a population of relatively young, hot stars. A central bulge is visible, although it appears somewhat subtle and elongated along the plane of the disk, lacking a distinct spherical shape. The outer regions of the disk fade gradually, indicating a smooth distribution of stellar density. No distinct spiral arms are discernible. The overall morphology is indicative of a relatively quiescent galaxy with ongoing, but limited, star formation. There is no clear indication of recent or ongoing major merger activity, although minor disturbances cannot be ruled out at this resolution.
