The galaxy appears as a largely featureless, elliptical structure, with a smooth light distribution. Its shape is somewhat elongated, though tending towards roundness. The galaxy exhibits a concentrated central region, with light intensity decreasing gradually towards its outer edges. No distinct spiral arms, bars, or dust lanes are discernible. The color is primarily yellowish-white, suggesting a dominant population of older stars. There is no visual evidence of ongoing major merger activity, though minor disturbances may be present but are difficult to discern due to the galaxy's smooth appearance. The galaxy's overall morphology is consistent with a passively evolving system, likely a massive elliptical galaxy.
