The galaxy presents as an elongated, disk-shaped structure, viewed at a significant inclination. There is a smooth, central bulge, appearing whitish and concentrated, which seems to dominate the light emission. Extending from the bulge along the major axis of the disk, there are regions of bluish light on one side of the galaxy and reddish light on the other side, suggesting differential stellar populations or dust extinction. There are no apparent spiral arm structures easily discernible. Some subtle irregular features seem to be present, with a slight warping along the galaxy disk. The lack of defined spiral arms indicates the galaxy is most likely smooth, with perhaps some disturbance evident within the disk structure. The overall color profile suggests ongoing, albeit low, star formation within the disk, particularly on one side, contrasting the older, redder population, seen on the other.
