The galaxy presents a largely smooth and rounded morphology, appearing elliptical in shape. A concentrated central bulge exhibits a bright, relatively uniform intensity suggesting a high stellar density. The luminosity decreases gradually from the center outwards, fading into the background sky. There is a subtle color gradient; the core appears slightly redder, while the outer regions exhibit a bluer tint. No distinct spiral arm structures or prominent dust lanes are discernible. There is a hint of minor disturbance or interaction visible, but it is generally a well-defined system. Based on the relatively smooth appearance, this galaxy may be an elliptical galaxy with a relatively small amount of star formation.
