The galaxy presents a primarily smooth morphology, displaying minimal discernible features such as spiral arms or a prominent central bulge. Its overall shape is somewhat elliptical, appearing neither perfectly spherical nor significantly elongated. The galaxy exhibits a color gradient, transitioning from a bluer hue in its central regions to redder tones towards its outer edges. This color variation suggests a central concentration of younger, hotter stars, while the outer regions potentially contain older, cooler stellar populations. There is a subtle indication of a possible minor disturbance or interaction influencing the galaxy's overall structure, though the evidence remains relatively weak. No strong indications of active star formation regions are apparent within the galaxy.
