The galaxy presents a generally smooth morphology, with a slight elongation suggesting an elliptical shape or a disk viewed at an angle. The light distribution is centrally concentrated, fading towards the edges. There may be a faint disk component; however, it is difficult to discern due to the galaxy's inclination and the image's resolution. Color gradients are subtle but present; the central region appears redder, which could indicate an older stellar population, while the outer regions show bluer hues. The galaxy displays no visible signs of major disturbances or ongoing merging events.
