The galaxy exhibits a flattened, elliptical morphology, suggesting it may be either an elliptical galaxy or a spiral galaxy viewed edge-on. The central region appears more concentrated and brighter than the outer regions. There is some indication of bluer colors concentrated near the edges of the disk, and a more red hue concentrated in the center. This color variation could point to areas of more recent star formation, if it is indeed a spiral galaxy. There is no visible bar structure or well-defined spiral arms, nor obvious signs of ongoing major mergers, although some degree of gravitational disturbance or interaction cannot be ruled out.
